#
# Aladin strings not so frequently used
#

# UCD1
AT	Atomic Data
AT_COLL	Atomic Collisional Quantities
AT_COLL_EXCIT-RATE	Collisional Excitation Rate
AT_COLL_STRENGTH	Collisional strength
AT_CONFIG	Electronic Configuration
AT_CONSTANT	Atomic Constant
AT_DAMPING	Atomic Damping Quantities
AT_DAMPING_VDWAALS	Van der Waals damping
AT_DATA	Various Atomic data
AT_DEGENERACY	Atomic Degeneracy Parameter
AT_DIPOLE	Atomic Dipole
AT_DIPOLE_MISC	Atomic Dipole
AT_DIPOLE_MOMENT	Atomic Dipole Momentum
AT_EIGENVECTOR	Atomic Eigenvector
AT_ELEC-COEFF	Atomic Electric Coefficient
AT_ELEMENT	Atomic Element Name
AT_EMISSIVITY	Atomic Emissivity
AT_ENERGY	Atomic Energy or Potential
AT_ENERGY_BAND	Atomic (molecular) Energy Band
AT_ENERGY_DIFF	Energy difference between experimental and calculated quantities
AT_ENERGY_EXCIT	Excitation Energy
AT_ENERGY_IONIZ	Ionization Energy or Potential
AT_ENERGY_LEVEL	Energy Level
AT_ENERGY_POTENTIAL	Atomic Energy or Potential
AT_ENERGY_ROTATION	Rotation Energy
AT_ENERGY_FORMATION	Formation energy (or heat for molecules)
AT_FREQUENCY	Transition Frequency
AT_FREQUENCY_NU	Transition Frequency at rest
AT_FREQUENCY_ROTAT	Rotation Frequency
AT_FS	Fine Structure Quantities
AT_FS_COLL-STR	Fine Structure Collision Strength
AT_FS_CONSTANT	Fine Structure Constant
AT_FS_CONTRIB	Fine Structure Contribution to Line Profile
AT_FS_SPLIT	Fine Structure Splitting
AT_GA	Atomic ga value
AT_INTENSITY	Line Intensity
AT_ION	Ions
AT_ION_ID	Ion Identification
AT_ION_STAGE	Ionization Stage
AT_LANDE-FACT	Lande Factor (gf)
AT_LEVEL	Level Identification
AT_LIFETIME	Radiative Lifetime
AT_LINE	Atomic or Molecular Lines
AT_LINE_EMISSIVITY	Line Emissivity
AT_LINE_FLUOR-YIELD	Line Fluorescence Yield
AT_LINE_ID	Line Identification
AT_LINE_STRENGTH	Line Strength
AT_MAIN-TERM	Main Term
AT_MOL	Quantities Related to Molecules
AT_MOL_DIEL-FN	Molecular Dielectric Function
AT_MOL_DISS-ENRGY	Molecular Dissociation Energy
AT_MOL_ID	Molecule Identification
AT_MOL_LEVEL	Molecule Transition Level
AT_MULTIPLET	Quantities Related to Multiplets
AT_MULTIPLET_ID	Multiplet Identification
AT_MULTIPLET_N	Multiplet Number element
AT_NUMBER	Atomic Number
AT_OSC	Oscillator Related Quantities
AT_OSC_STRENGTH	Oscillator Strength
AT_PARITY	Atomic Parity
AT_Q-N	Atomic Structure, Quantum Numbers
AT_Q-N_ANG-MOM	Angular Momentum Quantum Number
AT_Q-N_K	K quantum number
AT_Q-N_MISC	Atomic Structure Quantum Number
AT_Q-N_ORBITAL	Orbital Quantum Number
AT_Q-N_PRINCIPAL	Principal Quantum Number
AT_Q-N_PRINCIPAL_FIRST	First Principal Quantum Number
AT_Q-N_PRINCIPAL_SECOND	Second Principal Quantum Number
AT_Q-N_ROTATIONAL	Rotational Quantum Number
AT_Q-N_TORSIONAL	Torsional Quantum Number
AT_Q-N_VIBRATIONAL	Vibrational Quantum Number
AT_REACTION	Atomic Reaction
AT_SHELL-NUMBER	Shell Quantum Numbers
AT_SPECIES	Atomic Species Participating in a Reaction
AT_STARK	Stark Effect
AT_STARK_BROAD	Broadening due to Stark Effect
AT_STARK_INTENSITY	Intensity due to Stark Effect
AT_STAT-WEIGHT	Statistical Weight
AT_STRENGTH-PARAM	Strength Parameter or Expect Width
AT_TRANS	Quantities Related to Transitions
AT_TRANS_ENERGY	Transition Energy (or wavenumber)
AT_TRANS_ID	Transition Identification
AT_TRANS_LEVELS	Transition Level
AT_TRANS_PROB	Transition Probability
AT_TRANS_STRENGTH	Transition Strength
AT_TRANS_TYPE	Transition Type
AT_TRANS_RECOMBIN	Recombination coefficients in atomic transitions
AT_WAVELENGTH	Line Wavelength
AT_WEIGHT	Atomic Weight
CLASS	Various Classification Descriptors
CLASS_CODE	Classification Code
CLASS_COLOR	Color Classification
CLASS_DISTANCE	Abell Distance Class
CLASS_MISC	Various Classification Descriptors
CLASS_OBJECT	Object Type Classification
CLASS_RICHNESS	Abell Richness Class
CLASS_STAR/GALAXY	Star galaxy discriminator or classification.
CLASS_STRUCT	Structure Classification (e.g. cluster Bautz-Morgan classification)
CODE	Codes or Flags
CODE_ERROR	Flag denoting uncertainty about a given quantity
CODE_LIMIT	Lower or Upper limit Flag
CODE_MEMB	Membership Code
CODE_MISC	Miscellaneous Codes or Flags
CODE_MULT_FLAG	A code or flag indicating a multiplicity of binarity
CODE_MULT_FREQUENCY	Multiplicity Frequency Code
CODE_MULT_INDEX	Multiplicity Index Code
CODE_QUALITY	Quality Code
CODE_VARIAB	Variability Code or Flag
DATA	Quantities Related to the Data
DATA_FACTOR-EXP	Scale Factor Exponent (Base 10)
DATA_SCALE-FACTOR	Factor to Convert a Data Column to a normal value
DATA_TYPE	Data Type
CLASS_BRIGHT	Brightness class or code
DYN	Dynamic Data Quantities (mixed column content)
DYN_QUANTITY	Used when a Column means more than one thing.
DYN_VALUE	Identification of a Dynamic Value
ERROR	Error or Uncertainty in Measurements
EXTENSION	Quantities used to describe the extension in the sky of objects
EXTENSION_AREA	Angular Area Covered by an Object
EXTENSION_DEC	Angular Extension in Declination
EXTENSION_DIAM	Angular Diameter or Size of the Major Axis
EXTENSION_FWHM	Angular Full Width at Half Maximum (FWHM)
EXTENSION_FWHM_CIRC	Angular Full Width at Half Maximum (FWHM)
EXTENSION_FWHM_MAJ	Angular FWHM along the Major Axis
EXTENSION_FWHM_MIN	Angular FWHM along the Minor Axis
EXTENSION_HALFINT	Angular Size at Half Intensity
EXTENSION_MIN	Angular Diameter of an object along the Minor Axis
EXTENSION_NORM	Angular diameter normalized to beam size
EXTENSION_RA	Angular extension in right ascension
EXTENSION_RAD	Angular radius of an object or Semi-major axis
EXTENSION_SC-LENGTH	Angular Scale Length (bulge or disk)
EXTENSION_SMIN	Angular size of Semi-Minor Axis
FIT	Fits of Models to Observational Data
FIT_ERROR	Fit Error
FIT_GOODNESS	Fit Goodness
FIT_ID	Identification of the fit or solution
FIT_LF_GENERAL	Fit of Luminosity Function
FIT_LF_MAG	Magnitudes related to the LF
FIT_LF_MAG_MAX	Magnitude interval upper limit
FIT_LF_MAG_MIN	Magnitude interval lower limit
FIT_RATIO	Ratio of Measurement to Theoretical Value
FIT_PARAM_COVAR	Covariance of the fitting parameter
FIT_PARAM_ID	Fit Parameter Identification
FIT_PARAM_VALUE	Miscellaneous fit parameters
FIT_RESIDUAL	Fit Residual
FIT_CHI2	Chi-square Fit Measurement
FIT_STDEV	Fit's Standard Deviation
FIT_TYPE	Fit or Solution Type
FIT_ZP	Fit Zero Point (mostly in linear fits)
ID	Fields Used as Identifiers
ID_ALTERNATIVE	Alternative identification
ID_AREA	Area Identification (usually in a photographic plate)
ID_VERSION	Identification of the software version
ID_ASSOCIATED	Identification of Associated Object (counterpart)
ID_AUTHOR	Author Name
ID_CANDIDATE	Candidate Identification
ID_CATALOG	Catalog Identification
ID_CHART	Finding Chart Identification
ID_COMPARISON	Name of a Comparison Object
ID_CONSTEL	Constellation Name
ID_CROSSID	Cross Identification (counterpart)
ID_DATABASE	Database Identification
ID_DATASET	Data-Set Identification
ID_EXPOSURE	Exposure Identification
ID_FIBER	Fiber Optics Identification (for M.O.S.)
ID_FIELD	Field Identification
ID_FIGURE	Figure Identification Number
ID_FILE	File Identification
ID_FRAME	Frame Identification
ID_GROUP	Group Identification
ID_HUMAN	Identification of Discoverer or Observer
ID_IDENTIFIER	Identification of a source or object, incomplete or for internal use
ID_IMAGE	Image Identification
ID_MAIN	Main Identifier of a Celestial Object
ID_MAIN:1	First component of an identification field.
ID_MAIN:2	Second component of an identification field.
ID_MAIN:3	Third component of an identification field.
ID_MAP	Map Identification
ID_NUMBER	Numeric Identification (usually sequential)
ID_PARENT	Parent Identification (galaxy, cluster, nebulae)
ID_PLATE	Plate Identification
ID_REGION	Region or Zone Identification (not necessarily sky region)
ID_SET	Set or Subset Identification
ID_SITE	Site/Location/Observatory/City/Country identifier
ID_SLIT	Slit Identification (usually in the context of M.O.S.)
ID_SURVEY	Survey Identification
ID_TABLE	Table Identification
ID_TARGET	Target Indentifier
ID_PARAM	Identification or name of a parameter, or the name of a column in a table
ID_VARIAB	Variable Object Identification
INST	Instrumental Quantities
INST_ANG	Angular Properties of the Instruments/Telescopes
INST_ANG_OFFAXIS	Off-axis angle respect to main direction of observation
INST_ANG_PHASE	Satellite phase angle
INST_ANG_RESOL	Angular resolution of instrument
INST_ANG_VEL	Satellite angular velocity
INST_ANTENNA-TEMP	Antenna temperature
INST_APERT	Instrument/telescope aperture
INST_AREA	Collecting area or detector area
INST_BACKGROUND	Background contribution
INST_BAND	Instrumental Band quantities
INST_BAND_DRIFT	Band's drift rate
INST_BAND_PASS	Bandpass
INST_BANDWIDTH	Spectral window used for the observation
INST_BASELINE	Baseline (interferometry)
INST_BEAM	Beam properties
INST_BEAM_MISC	Miscellaneous beam properties
INST_BEAM_SIZE	Beam width or size
INST_BEAM_TEMP	Beam temperature
INST_CALIB	Intstrument calibration quantities
INST_CALIB_ERROR	Instrument calibration error
INST_CALIB_MISC	Miscellaneous instrument calibration quantities
INST_CALIB_PARAM	Calibration parameter
INST_CORR-FACTOR	Correction factor
INST_DET	Detector parameters
INST_DET_LIMIT	Detector limit
INST_DET_MISC	Miscellaneous quantities related to the detector (plate or CCD)
INST_DET_SIZE	Detector size
INST_DISPERSION	Dispersion scale in a spectrograph
INST_EFFICIENCY	Instrument efficiency
INST_ERROR	Errors associated to the instrument
INST_FILTER	Filter characteristics
INST_FILTER_CODE	Filter characteristics type/code
INST_FILTER_FWHM	FWHM of the used filter (also bandpass)
INST_FILTER_TRANSM	Transmission characteristics of the filter (response)
INST_ID	Instrument/Detector Identification
INST_LINE-WIDTH	Instrumental Line-Width
INST_NOISE	Detector/Instrument noise level rms
INST_PARAM	Various Instrumental Parameters
INST_PIXSIZE	Pixel Size
INST_PLATE	Quantities related to Photographic Plates
INST_PLATE_DIMENSION	Size or plate dimension
INST_PLATE_DIST	Distance measurement on a plate
INST_PLATE_EMULSION	Plate Emulsion Type
INST_PLATE_EXTENSION	Extension of an object in a plate (in plate units)
INST_POS	Position on a detector or M.O.S template
INST_PRECISION	Instrumental Precision
INST_PSF	Detector's Point Spread Function (PSF)
INST_QE	Detector's Quantum Efficiency
INST_S/N	Instrumental signal to noise ratio (S/N)
INST_SAMP-TIME	Instrumental Sampling Time
INST_SCALE	Instrumental Scale (ccd or plate)
INST_SEEING	Seeing or fwhm of PSF
INST_SENSITIVITY	Detector's Sensitivity (Flux limit)
INST_SETUP	Instrument configuration or setup
INST_SKY_SIGMA	Sigma of sky value distribution
INST_SKY_LEVEL	Local Sky Level
INST_SKY_TEMP	Sky Temperature
INST_SPECT	Spectroscopic instruments' quantities
INST_SPECT_BAND	Spectroscopic observation band
INST_SPECT_ORDER	Spectral Order
INST_SPECT_SLIT-LENGTH	Slit Length
INST_SPECT_SLIT-WIDTH	Slit Width
INST_TEMP	Instrument Temperature (radio regime)
INST_TEMP_SYST	System Temperature
INST_TRIGGER	Detector's triggering Threshold
INST_TYPE	Instrument Type
INST_VELOC	Velocity Quantities at the Instrumental Level
INST_VELOC_CENTRAL	Instrumental Central Velocity
INST_VELOC_SPACING	Instrumental Velocity Channel Spacing
INST_VELOC_WINDOW	Detector's Velocity Range
INST_WAVELENGTH	Observation's Wavelength properties
INST_WAVELENGTH_COVERAGE	Instrument's Wavelength Range
INST_WAVELENGTH_EFFECTIVE	Observation's Effective Wavelength
INST_SPECT_CODE	Spectroscopic instrument specification (prism, grism, grating)
LUNAR-OCCULT	Lunar Occultation related quantities
LUNAR-OCCULT_ANGLE	Lunar Occultaion Contact Angle
LUNAR-OCCULT_LIMB-SLOPE	Lunar Occultation Limb Slope
MODEL	Quantities generated by Models
MODEL_CONTINUUM	Continuum level
MODEL_CORRECTION	Correction or adjustment
MODEL_DRIFT-VELOC	Terminal drift velocity
MODEL_DYN-TRIAX	Dynamical triaxiality
MODEL_ENERGY	Energy modelled quantities
MODEL_ENERGY_DIST	Energy distribution
MODEL_EOS	Equation of state
MODEL_EOS_ID	Name of used equation of state
MODEL_EXTINCTION	Insterstellar extinction quantitites
MODEL_EXTINCTION_COEFF	Interstellar extinction coefficient
MODEL_FEATURE	Model Feature
MODEL_FLUX	Modelled Flux
MODEL_ID	Model Identification
MODEL_LINE-FLUX	Model Spectral Line Flux
MODEL_MAG	Model-generated Magnitude
MODEL_MAG_CORR	Magnitude Correction or Difference
MODEL_PARAM	Model Parameter
MODEL_POP-SYNTHESIS	Population Synthesis Quantity
MODEL_RESIDUAL	Model Residual
MODEL_RESULT	Model Solution Value
MODEL_TYPE	Model Type
MODEL_ZEEMAN	Zeeman Effect Quantities
MODEL_ZEEMAN_COEFF	Zeeman Effect Coefficient
MORPH	Morphology of celestial objects
MORPH_ARMS	Spiral Arms Structure (galaxies)
MORPH_ARMS_RATIO	Ratio of Spiral Arm (galaxies)
MORPH_ARMS_WOUND	Wound Parameter of a spiral arm galaxy
MORPH_ASYMMETRY	Asymmetry Induced by Rotation
MORPH_BAR	Presence or detection of a bar in a galaxy
MORPH_CODE	Code refering to a morphological property
MORPH_PARAM	Morphological (geometrical) parameter
MORPH_TYPE	Morphological Type
NOTE	A Note related to a certain quantity or value
NUMBER	Number Of ``things'' (stars, observations, etc.)
NUTATION	Earth's Nutation Related Quantities
NUTATION_PARAM	Nutation Parameter
OBS	Observational Quantities
OBS_ANG-SIZE	Observational angular size
OBS_BAND	Band or Filter used for the observation
OBS_CALIB	Calibrations related to observations
OBS_CALIB_CONST	Calibration's Constant
OBS_CALIB_FACTOR	Calibration conversion factor
OBS_CODE	Observation code for observing run
OBS_CONDITIONS	Observation condition
OBS_DETECT-LIMIT	Detection Limit
OBS_DETECT-SIGNIF	Detection Significance
OBS_DIFF	Observations' offset, difference, or deviation
OBS_DRIFT	Positional drift during the observation
OBS_FREQUENCY	Frequency of the observation
OBS_ID	Observation identification
OBS_LW	Observed gaussian line-width
OBS_METHOD	Observational Method/Technique
OBS_OTHER	Other Measurements
OBS_PARAM	Additional Observational Parameters
OBS_PLATE	Quantities related to measurements on plates
OBS_PLATE_APERT	Plate (Circular) Aperture
OBS_PLATE_EXTENSION	Linear diameter of an object measured on a Plate
OBS_PRED/OBS	Fraction of predicted to observed quantities
OBS_RUN	Observation run
OBS_SIZE	Observed size
OBS_SIZE_DEC	Observed size in declination
OBS_SLIT	Spectroscopic slit properties
OBS_SLIT_OFFSET	Slit offset respect to the nucleus of galaxy
OBS_SLIT_ORIENT	Slit orientation
OBS_SPECTRUM	Spectral observations
OBS_TYPE	Type of observation
OBSTY	Data on Observatories
OBSTY_ALTITUDE	Observatory Altitude
OBSTY_CODE	Observatory Code
OBSTY_ID	Observatory Identification/Name
ORBIT	Orbital elements (planets, double stars, galaxies)
ORBIT_ASC-NODE	Longitude of ascending node
ORBIT_COMETS	Cometary orbit parameter
ORBIT_CONV-ANGLE	Convergence angle
ORBIT_DISTANCE	Distance, perihelion, or separation between components
ORBIT_ECCENTRICITY	Orbital eccentricity
ORBIT_ELONGATION	Elongation of radiant
ORBIT_FREQUENCY	Orbital frequency (orbital angular velocity)
ORBIT_MEAN-ANOMALY	Mean anomaly
ORBIT_P-ASTRON	Quantities related to the Periastron
ORBIT_P-ASTRON_ARG	Periastron argument or longitude
ORBIT_P-ASTRON_DATE	Date of occurance of periastron
ORBIT_P-ASTRON_RATE	Rate of periastron advance
ORBIT_P-HELION	Perihelion argument or longitude
ORBIT_PARAM	Orbital parameter
ORBIT_PERIOD	Orbital period
ORBIT_PERIOD_DERIVATIVE	Time derivative of orbital period
ORBIT_PHASE-ANGLE	Orbital phase angle
ORBIT_RV	Orbital radial velocity properties
ORBIT_RV_S-AMPLITUDE	Semi amplitude of radial velocity curve
ORBIT_SEPARATION	Orbital Separation (angular distance)
ORBIT_SIZE	Orbital size
ORBIT_SIZE_RADIUS	Orbital radius (binary stars)
ORBIT_SIZE_SMAJ	Semi-major axis of the orbit
PHOT	Photometry, extending to several wavelength regimes (X to Radio)
PHOT_13C	13 color system (Stellar Applications) GCPD#66
PHOT_13C_33-52	Color index 33-52 (13C)
PHOT_13C_35-52	Color index 35-52 (13C)
PHOT_13C_37-52	Color index 37-52 (13C)
PHOT_13C_40-52	Color index 40-52 (13C)
PHOT_13C_45-52	Color index 45-52 (13C)
PHOT_13C_52	Magnitude 52 (13C)
PHOT_13C_52-110	Color index 52-110 (13C)
PHOT_13C_52-58	Color index 52-58 (13C)
PHOT_13C_52-63	Color index 52-63 (13C)
PHOT_13C_52-72	Color index 52-72 (13C)
PHOT_13C_52-80	Color index 52-80 (13C)
PHOT_13C_52-86	Color index 52-86 (13C)
PHOT_13C_52-99	Color index 52-99 (13C)
PHOT_ABS-MAG	Absolute magnitude
PHOT_ABS-MAG_BAND	Absolute magnitude in a band, regardless of band
PHOT_ABS-MAG_BOL	Bolometric absolute magnitude
PHOT_ATM	Earth Atmosphere Parameters Linked to Photometry
PHOT_ATM_AIRMASS	Air mass
PHOT_ATM_EXT	Atmospheric extinction coefficient
PHOT_BOL	Bolometric Quantities
PHOT_BOL_CORR	Bolometric correction
PHOT_BOL_FLUX	Bolometric Flux
PHOT_BOL_LUMINOSITY	Bolometric luminosity
PHOT_BOL_MAG	Bolometric magnitude
PHOT_BRIGHTNESS-SLOPE	Spatial brightness distribution slope
PHOT_CI	Color index in unspecified system
PHOT_CI_102-C220	Color index 102-C220
PHOT_CI_B-R	Color index B-r
PHOT_CI_B-V	Color index B-V in a non-conventional system
PHOT_CI_BETA	Color index beta or h-beta
PHOT_CI_B-I	Color index B-I from heterogeneous photometric systems
PHOT_CI_B-K	Color index B-K from heterogeneous photometric systems
PHOT_SDSS_U-G	Color index u'-g' from SDSS (Sloan Digital Sky Survey)
PHOT_SDSS_G-R	Color index g'-r' from SDSS (Sloan Digital Sky Survey)
PHOT_SDSS_R-I	Color index r'-i' from SDSS (Sloan Digital Sky Survey)
PHOT_CI_CN-TIO	Color index CN-TiO
PHOT_CI_CODE	Codes associated with color index
PHOT_CI_GB-GV	Color index gb-gv
PHOT_CI_GU-GB	Color index gu-gb
PHOT_CI_IR-OPT	Color index Infrared minus optical
PHOT_CI_M-51	Color index M-51
PHOT_CI_R-HALPHA	Color index R minus Halpha
PHOT_CI_R-I	Color index R-I
PHOT_CI_U-B	Color index u-B
PHOT_SDSS_I-Z	Color index i'-z' in  Sloan Digital Sky Survey system (1996AJ....111.1748F)
PHOT_CI_U-R	Color index u-r
PHOT_CI_UNDEF	Color index in unspecified system
PHOT_CI_UV-OPT	Color index uv minus Optical (UV-OPT)
PHOT_CI_V-I	Color index V-I (no standard system specified)
PHOT_CI_V-R	Color index V-R (no standard system specified)
PHOT_CLASS	Classification of photometry
PHOT_COLOR	Quantities related to color indices
PHOT_COLOR_EXCESS	Color excess (not just E(B-V))
PHOT_COUNT-RATE	Count rates in several wavelength regimes
PHOT_COUNT-RATE_UV	Count rate in ultraviolet
PHOT_COUNT-RATE_X	Count rate in x-ray
PHOT_COUNTS	Count measured in the detector
PHOT_COUNTS_IUE	Count from IUE
PHOT_COUNTS_MISC	Count measurement in the detector
PHOT_COUNTS_RADIO	Counts in radio regime
PHOT_COUNTS_GAMMA	Count in gamma-ray regime
PHOT_COUNT-RATE_GAMMA	Count rate of gamma photons
PHOT_COUNTS_RATIO	Ratio of photon counts, or relative counts
PHOT_COUNTS_X	Counts in X-ray
PHOT_COUS	Cousins photometric system GCPD#54
PHOT_COUS_I	Cousins magnitude I COUS
PHOT_COUS_R	Cousins magnitude R COUS
PHOT_COUS_R-I	Cousins R-I color index COUS
PHOT_COUS_V-I	(Kron-)Cousins V-I color index COUS
PHOT_COUS_V-R	(Kron-)Cousins V-I color index
PHOT_DDO	DDO Photometric System GCPD#12
PHOT_DDO_48-51	Color index 48-51 in DDO
PHOT_DDO_38-41	Color index 38-41 DDO
PHOT_DDO_41-42	Color index 41-42 DDO
PHOT_DDO_42-45	Color index 42-45 DDO
PHOT_DDO_42-48	Color index 42-48 DDO
PHOT_DDO_45-48	Color index 45-48 DDO
PHOT_DDO_M48	Magnitude m48 DDO
PHOT_DIFF	Differences or differential quantities
PHOT_DIFF_CI	Difference in color index
PHOT_DIFF_MAG	Difference in or differential magnitude
PHOT_DIFF_SB	Difference in surface brightness
PHOT_DIST-MOD	Distance Modulus
PHOT_EXTINCTION	Extinction total to differential
PHOT_EXTINCTION_GAL	Galactic extinction
PHOT_EXTINCTION_INT	Internal extinction
PHOT_EXTINCTION_ISM	Interstellar Absorption
PHOT_EXTINCTION_R	Interstellar extinction (ratio total to differential)
PHOT_EXTINCTION_TOTAL	Total Extinction
PHOT_FLUENCE	Fluence
PHOT_FLUX	Flux
PHOT_FLUX_DENSITY	Flux density
PHOT_FLUX_GAMMA	Flux in gamma rays
PHOT_FLUX_HALPHA	H-Alpha Flux
PHOT_FLUX_IR_15	IR flux around 15{mu}m
PHOT_FLUX_IR	IR flux (IRAS or others)
PHOT_FLUX_IR_100	Flux density (IRAS) at 100 microns
PHOT_FLUX_IR_12	Flux density (IRAS) at 12 microns
PHOT_FLUX_IR_25	Flux density (IRAS) at 25 microns
PHOT_FLUX_IR_3.5	Flux density at 3.5 microns
PHOT_FLUX_IR_60	Flux density (IRAS) at 60 microns
PHOT_FLUX_IR_FAR	Far Infrared flux
PHOT_FLUX_IR_H	Flux Density in Johnson's H Band
PHOT_FLUX_IR_L	Flux Density in Johnson's L Band
PHOT_FLUX_IR_MISC	Miscellaneous IR fluxes
PHOT_FLUX_NORM	Normalized Flux, always dimensionless
PHOT_FLUX_OPTICAL	Flux in the Optical (unspecified system and/or units)
PHOT_FLUX_RADIO	Flux density at radio frequencies
PHOT_FLUX_RADIO_22M	Radio Flux density around 22MHz (13.6m)
PHOT_FLUX_RADIO_31M	Radio flux density around 31MHz (9.7m)
PHOT_FLUX_RADIO_43M	Radio flux density around 43MHz (7.0m)
PHOT_FLUX_RADIO_61M	Radio flux density around 61MHz (4.9m)
PHOT_FLUX_RADIO_87M	Radio flux density around 87MHz (3.5m)
PHOT_FLUX_RADIO_110M	Radio flux density around 110MHz (2.7m)
PHOT_FLUX_RADIO_150M	Radio flux density around 150MHz (2.0m)
PHOT_FLUX_RADIO_175M	Radio flux density around 175MHz (1.7m)
PHOT_FLUX_RADIO_250M	Radio flux density around 250MHz (1.2m)
PHOT_FLUX_RADIO_325M	Radio flux density around 325MHz (92cm)
PHOT_FLUX_RADIO_365M	Radio flux density around 365MHz (82cm)
PHOT_FLUX_RADIO_400M	Radio flux density around 400MHz (75cm)
PHOT_FLUX_RADIO_500M	Radio flux density around 500MHz (60cm)
PHOT_FLUX_RADIO_600M	Radio flux density around 600MHz (50cm)
PHOT_FLUX_RADIO_700M	Radio flux density around 700MHz (43cm)
PHOT_FLUX_RADIO_850M	Radio flux density around 850MHz (35cm)
PHOT_FLUX_RADIO_1G	Radio flux density around 1GHz (30cm)
PHOT_FLUX_RADIO_1.4G	Radio flux density around 1.4GHz (21cm)
PHOT_FLUX_RADIO_1.6G	Radio flux density around 1.6GHz (19cm) (OH maser)
PHOT_FLUX_RADIO_2G	Radio flux density around 2GHz (15cm)
PHOT_FLUX_RADIO_2.7G	Radio flux density around 2.7GHz (11cm)
PHOT_FLUX_RADIO_3.9G	Radio flux density around 3.9GHz (7.7cm)
PHOT_FLUX_RADIO_5G	Radio flux density around 5GHz (6cm)
PHOT_FLUX_RADIO_7.5G	Radio flux density around 7.5GHz (4cm)
PHOT_FLUX_RADIO_8.4G	Radio flux density around 8.4GHz (3.6cm)
PHOT_FLUX_RADIO_10.7G	Radio flux density around 10.7GHz (2.8cm)
PHOT_FLUX_RADIO_15G	Radio flux density around 15GHz (2cm)
PHOT_FLUX_RADIO_22G	Radio flux density around 22GHz (13.6mm) (H2O maser)
PHOT_FLUX_RADIO_36G	Radio flux density around 36GHz (8.3mm)
PHOT_FLUX_RADIO_43G	Radio flux density around 43GHz (7.0mm)
PHOT_FLUX_RADIO_63G	Radio flux density around 63GHz (4.8mm)
PHOT_FLUX_RADIO_90G	Radio flux density around 90GHz (3.3mm)
PHOT_FLUX_RADIO_125G	Radio flux density around 125GHz (2.4mm)
PHOT_FLUX_RADIO_180G	Radio flux density around 180GHz (1.7mm)
PHOT_FLUX_RADIO_250G	Radio flux density around 250GHz (1.2mm)
PHOT_FLUX_RADIO_350G	Radio flux density around 350GHz (860um)
PHOT_FLUX_RADIO_500G	Radio flux density around 500GHz (600um)
AT_ENERGY_TOTAL	Total Energy
AT_TRANS_BRNCH-RATIO	Transition branching ratio
DATA_LINK	Link to correlated data
DATA_MAXIMUM	Maximal value of some parameter in an array or series
INST_WAVELENGTH_VALUE	Instrumentation wavelength
MODEL_MAG_VALUE	magnitude from a model
PHOT_DDO_35-38	Color index 35-38 in DDO system
PHOT_FLUX_HBETA	Flux in H-beta line
PHOT_FLUX_RADIO_700G	Radio flux density around 700GHz (430um)
PHOT_HST_CI_R-I	HST Color Index close to R-I, e.g. F675W-F814W
PHOT_CI_ALPHA	Color index based on H-alpha line
PHOT_CI_BALMER	Color index using the Balmer lines Hgamma or higher
PHOT_INT-BAND_U	Intermediate photometry bands in near-UV (300-400nm)
PHOT_INT-BAND_B	Intermediate photometry bands in blue region (400-500nm)
PHOT_INT-BAND_V	Intermediate photometry bands in visible region (500-600nm)
PHOT_INT-BAND_R	Intermediate photometry bands in red region (600-800nm)
PHOT_INT-BAND_I	Intermediate photometry bands in near-IR region (800-1000nm)
PHOT_INT-MAG_K	Integrated, total or isophotal, K magnitude
PHOT_INT-MAG_H	Integrated, total or isophotal, H magnitude
PHOT_INT-MAG_J	Integrated, total or isophotal, K magnitude
PHOT_INT-MAG_U	Integrated, total or isophotal, U magnitude
PHOT_INT-MAG_I	Integrated, total or isophotal, I magnitude
REDSHIFT_PHOT	Photometric redshift
SPECT_LINE_DIFF-FREQ	Differential frequency between two lines (usually in radio)
PHOT_FLUX_RADIO_MISC	Miscellaneous Radio flux density, e.g. Frequency given in another column
PHOT_FLUX_RADIO_SIO-MASER	SiO maser peak radio flux
PHOT_FLUX_RATIO	Flux ratio
PHOT_FLUX_REL	Relative (normalized) flux
PHOT_FLUX_UV	Ultraviolet flux (uv far-uv euv)
PHOT_FLUX_X	X-ray flux
PHOT_GEN_MISC	Miscellaneous Geneva Photometry indices
PHOT_GEN_B-V	Geneva color index B-V (GEN)
PHOT_GEN_B1-B	Geneva color index B1-B (GEN)
PHOT_GEN_B1-B2	Geneva color index B1-B2
PHOT_GEN_B2-B	Geneva color index B2-B (GEN)
PHOT_GEN_DELTA	Geneva photometric index Delta = (U-B2) - 0.832(B2-G)
PHOT_GEN_G-B	Geneva color index G-B (GEN)
PHOT_GEN_M2	Geneva photometric index m2 = (B1-B2) - 0.457(B2-V1)
PHOT_GEN_U-B	Geneva color index U-B (GEN)
PHOT_GEN_V	Geneva magnitude filter V (GEN)
PHOT_GEN_V-B	Geneva color index V-B (GEN)
PHOT_GEN_V1-B	Geneva color index V1-B (GEN)
PHOT_GEN_V1-G	Geneva color index V1-G
PHOT_GUNN	Gunn Photometric System GCPD#38
PHOT_GUNN_G	Magnitude g (GUNN)
PHOT_GUNN_G-I	Color index g-i (GUNN)
PHOT_GUNN_G-R	Color index g-r (GUNN)
PHOT_GUNN_I	Magnitude i (GUNN)
PHOT_GUNN_I-Z	Color index I-z (GUNN)
PHOT_GUNN_R	Magnitude R (GUNN)
PHOT_GUNN_R-I	Color index R-I (GUNN)
PHOT_GUNN_V	Magnitude v (GUNN)
PHOT_GUNN_V-R	Color index V-R (GUNN)
PHOT_GUNN_Z	Magnitude z (GUNN)
PHOT_HEI	Heidelberg s Photometric System (HEI)
PHOT_HEI_U-B	Heidelberg photometry U-B (HEI)
PHOT_HIPPAR	Hipparcos' photometry system
PHOT_HST	HST Photometric System (by filter name) (HST)
PHOT_HST_F1042M	Magnitude F1042M (HST)
PHOT_HST_F140W	Magnitude M104W (HST)
PHOT_HST_CI_IR	HST Color Index from IR filters, e.g. F140W-F210W
PHOT_HST_CI_U-B	HST Color Index close to U-B, e.g. F336W-F430W
PHOT_HST_F170W	Magnitude F170W (HST)
PHOT_HST_F175W	Magnitude F175W (HST)
PHOT_HST_F220W	Magnitude F220W (HST)
PHOT_HST_F255W	Magnitude F255W (HST)
PHOT_HST_F275W	Magnitude F275W (HST)
PHOT_HST_F300W	Ultraviolet Magnitude F300W (HST)
PHOT_HST_CI_U-V	HST Color Index close to U-V, e.g. F336W-F555W
PHOT_HST_F342W	Ultraviolet Magnitude in filters F330W or F342W (HST)
PHOT_HST_F430W	Ultraviolet magnitude F430W or F439W (HST)
PHOT_HST_CI_B-V	HST Color Index close to B-V, e.g. F430W-F555W
PHOT_HST_F450W	Ultraviolet Magnitude F450W (HST)
PHOT_HST_F480LP	Magnitude F480LP (HST)
PHOT_HST_F547M	Magnitude F547M (HST)
PHOT_HST_F555W	Magnitude F555W (HST)
PHOT_HST_CI_B-R	HST Color Index close to B-R, e.g. F430W-F675W
PHOT_HST_CI_V-R	HST Color Index close to V-R, e.g. F555W-F675W
PHOT_HST_F569W	Magnitude F569W (HST)
PHOT_HST_F606W	Magnitude F606W (HST)
PHOT_HST_CI_V-I	HST Color Index close to V-I, e.g. F555W-F814W
PHOT_HST_F622W	Magnitude F622W (HST)
PHOT_HST_F675W	Magnitude F675W (HST)
PHOT_HST_F702W	Magnitude F702W (HST)
PHOT_HST_F725LP	Magnitude F725LP (HST)
PHOT_HST_F785LP	Magnitude F785LP (HST)
PHOT_HST_F791W	Magnitude F791W (HST)
PHOT_HST_F814W	Magnitude F814W (HST)
PHOT_HST_F850LP	Magnitude F850LP (HST)
PHOT_HST_V	Magnitude V (visual) HST (unspecified filter name)
PHOT_INDX	Photometric index (usually in narrow bands)
PHOT_INDX_HI	Neutral hydrogen HI photometry index
PHOT_INT-MAG	Integrated magnitudes
PHOT_INT-MAG_B	Integrated, total or isophotal, B magnitude
PHOT_INT-MAG_MISC	Integrated (total or isophotal) magnitude
PHOT_INT-MAG_R	Integrated, total or isophotal, R magnitude
PHOT_INT-MAG_V	Integrated, total or isophotal, V magnitude
PHOT_INTENSITY	Intensity
PHOT_INTENSITY_ADU	Intensity expressed in ADU (analog to digital units)
PHOT_INTENSITY_ESTIMATED	Estimated intensity
PHOT_INTENSITY_MISC	Miscellaneous Intensity
PHOT_INTENSITY_NORMALIZED	Normalized intensity
PHOT_INTENSITY_PROFILE	Intensity profile
PHOT_INTENSITY_RATIO	Intensity ratio
PHOT_IR	Infrared magnitudes (not well inserted in photometric systems)
PHOT_IR_12-25	Infrared color index 12-25 (IRAS)
PHOT_IR_2.29	CO band index magnitude at 2.29 micron
PHOT_IR_25-60	Infrared IRAS color index 25-60 microns
PHOT_IR_3.4	Infrared magnitude at 3.4 microns
PHOT_IR_4.2	Infrared magnitude at 4.2 micron
PHOT_CI_IR	Various far IR color indices (e.g. with IRAS bands)
PHOT_IR_BGAMMA	Infrared Bracket Gamma magnitude
PHOT_IR_K-10	Infrared color index K-10 (K minus 10 microns)
PHOT_IR_K-100	Infrared color index K-100 (K minus 100 microns)
PHOT_IR_K-12	Infrared color index K-12 (K minus 12 microns)
PHOT_IR_K-25	Infrared color index K-25 (K minus 25 microns)
PHOT_IR_K-60	Infrared color index K-60 (K minus 60 microns)
PHOT_IR_L0	Infrared magnitude L at 3.7 micron
PHOT_IR_MAG	Far infrared magnitude mfir (may include IRAS bands)
PHOT_IR_N1:8.38	Infrared magnitude at 8.38 microns
PHOT_IR_N2:9.69	Infrared magnitude at 9.69 microns
PHOT_IR_N3:12.89	Infrared magnitude at 12.89 microns
PHOT_IR_N:10.4	Infrared magnitude N at 10.4 microns
PHOT_IR_Q:18.06	Infrared magnitude at 18.06 microns
PHOT_JHN	Johnson's Photometric system GCPD#8 GCPD#9
PHOT_JHN_B	Johnson magnitude B (JHN)
PHOT_JHN_B-H	Johnson color index B-H (JHN)
PHOT_JHN_B-I	Johnson color index B-I (JHN)
PHOT_JHN_B-K	Johnson color index B-K (JHN)
PHOT_JHN_B-K'	Johnson color index B-K' (JHN)
PHOT_JHN_B-R	Johnson color index B-R (JHN)
PHOT_JHN_B-V	Johnson color index B-V (JHN)
PHOT_JHN_H	Johnson magnitude H (JHN)
PHOT_JHN_H-K	Johnson color index H-K (JHN)
PHOT_JHN_I	Johnson magnitude I (JHN)
PHOT_JHN_I-K	Johnson color index I-K (JHN)
PHOT_JHN_J	Johnson magnitude J (JHN)
PHOT_JHN_J-H	Johnson color index J-H (JHN)
PHOT_JHN_J-K	Johnson color index J-K (JHN)
PHOT_JHN_K	Johnson magnitude K (JHN)
PHOT_JHN_K'	Johnson magnitude K' (JHN)
PHOT_JHN_K-L	Johnson color index K-L (JHN)
PHOT_JHN_K-L'	Johnson color index K-L' (JHN)
PHOT_JHN_K-M	Johnson color index K-M (JHN)
PHOT_JHN_K-N	Johnson color index K-N (JHN)
PHOT_JHN_K-Q	Johnson color index K-Q (JHN)
PHOT_JHN_L	Johnson magnitude L (JHN)
PHOT_JHN_L'	Johnson magnitude L' (JHN)
PHOT_JHN_L-M	Johnson color index L-M (JHN)
PHOT_JHN_M	Johnson magnitude M (JHN)
PHOT_JHN_MISC	Johnson Photometric system GCPD#8 GCPD#9
PHOT_JHN_N	Johnson flux magnitude N (JHN)
PHOT_JHN_R	Johnson magnitude R (JHN)
PHOT_JHN_R-H	Johnson color index R-H (JHN)
PHOT_JHN_R-I	Johnson color index R-I (JHN)
PHOT_JHN_R-K	Johnson color index R-K
PHOT_JHN_U	Johnson magnitude U (JHN)
PHOT_JHN_U-B	Johnson color index U-B (JHN)
PHOT_JHN_U-V	Johnson color index U-V (JHN)
PHOT_JHN_V	Johnson magnitude V (JHN)
PHOT_JHN_V-H	Johnson color index V-H (JHN)
PHOT_JHN_V-I	Johnson color index V-I (JHN)
PHOT_JHN_V-J	Johnson color index V-J (JHN)
PHOT_JHN_V-K	Johnson color index V-K (JHN)
PHOT_JHN_V-L	Johnson color index V-L (JHN)
PHOT_JHN_V-M	Johnson color index V-M (JHN)
PHOT_JHN_V-N	Johnson color index V-N (JHN)
PHOT_JHN_V-R	Johnson color index V-R (JHN)
PHOT_K-CORRECTION	K correction
PHOT_LCKWD	Lockwood photometric system GCPD#30
PHOT_LCKWD_81-78	Color index 81-78 LCKWD
PHOT_MAG	Magnitude of uncertain origin
PHOT_MAG_5007	Magnitude O III lambda 5007
PHOT_MAG_J	Near-Infrared magnitude around 1.2um (undefined or non-conventional system)
PHOT_MAG_B	Blue B magnitude
PHOT_MAG_CENTR	Central magnitude
PHOT_MAG_CORR	Magnitude correction
PHOT_MAG_H	Near-Infrared magnitude around 1.6um (undefined or non-conventional system)
PHOT_MAG_DROP	Drop in magnitude
PHOT_MAG_EYE	Eye estimated magnitude
PHOT_MAG_HI	Magnitude associated with neutral hidrogen
PHOT_MAG_I	Near-Infrared magnitude (undefined system)
PHOT_MAG_LIMIT	Magnitude limit
PHOT_MAG_OFFST	Magnitude offset
PHOT_MAG_OPTICAL	Optical magnitude
PHOT_MAG_R	Red (R) magnitude
PHOT_MAG_K	Near-Infrared magnitude around 2.2um (undefined or non-conventional system)
PHOT_MAG_U	U' magnitude (3402 A)
PHOT_MAG_UNDEF	Magnitude of uncertain origin or different bands in same column
PHOT_MAG_UV	Ultraviolet magnitude
PHOT_MAG_V	Visual magnitude
PHOT_PAL	Palomar Photometric System
PHOT_PHG_V-R	Photographic color index V-R (or g-r)
PHOT_PHG	Photographic magnitude Quantities
PHOT_PHG_B	Photographic blue magnitude B (includes the O magnitude of POSS)
PHOT_PHG_B-R	Photographic color index B-R (includes the O-E color index from POSS)
PHOT_PHG_B-V	Photographic color index B-V
PHOT_PHG_BJ	Photographic magnitude Bj
PHOT_PHG_BJ-RF	Photographic color index Bj-Rf
PHOT_PHG_F	Photographic magnitude F
PHOT_PHG_I	Photographic magnitude I
PHOT_PHG_U-B	Photographic color index U-B
PHOT_PHG_MAG	Photographic magnitude in unidentified band
PHOT_PHG_U	Ultraviolet photographic magnitude
PHOT_PHG_U-V	Photographic color index U-V
PHOT_PHG_R	Photographic red band magnitude R (includes E magnitude from POSS)
PHOT_PHG_R-I	Photographic color index R-I
PHOT_PHG_V	Photographic visual magnitude V
PHOT_PROFILE	Light distribution profile
PHOT_PROFILE_PAR	Light distribution's profile parameter
PHOT_RF_MISC	Miscellaneous reddening-free photometric indices
PHOT_RF_B-L	B-L extinction free color
PHOT_RF_B-U	B-U extinction free color
PHOT_RF_Q	Reddening free Q parameter
PHOT_RF_STR	Reddening free indices in the Stroemgren system
PHOT_RF_STR_C0	Dereddened color index parameter c0
PHOT_RF_STR_M0	Dereddened color index parameter m0
PHOT_RF_U-W	U-W extinction free color
PHOT_RF_V	Reddening free magnitude v
PHOT_RF_X	Reddening free geneva photometry parameter
PHOT_RF_Y	Reddening free geneva photometry parameter
PHOT_RF_Z	Reddening free geneva photometry parameter
PHOT_SB	Surface Brightness quantities
PHOT_SB_CI	Color index differential surface brightness
PHOT_SB_CODE	Encoded Surface Brightness
PHOT_SB_GENERAL	Surface Brightness (in general)
PHOT_SB_GUNN-G	Surface Brightness in Gunn G
PHOT_SB_IR-100	Surface Brightness at 100 micron
PHOT_SB_JHN	Surface Brightness in Johnson's System
PHOT_SB_JHN_B	Surface Brightness in Johnson B
PHOT_SB_JHN_B-R	Surface brightness Johnson's color B-R
PHOT_SB_JHN_H	Surface Brightness in Johnson H
PHOT_SB_JHN_I	Surface Brightness in Johnson I
PHOT_SB_JHN_J	Surface Brightness in Johnson J
PHOT_SB_JHN_K	Surface Brightness in Johnson K
PHOT_SB_JHN_K'	Surface Brightness in Johnson K'
PHOT_SB_JHN_R	Surface Brightness in Johnson R
PHOT_SB_JHN_U	Surface Brightness in Johnson U
PHOT_SB_JHN_U-R	Surface Brightness color idex U-R
PHOT_SB_JHN_V	Surface Brightness in johnson V
PHOT_SB_LIMIT	Surface Brightness Limit
PHOT_SB_RATIO	Surface Brightness Ratio, typically bulge/total for a galaxy
PHOT_SB_SKY	Sky Surface Brightness
PHOT_SD/B-BRIGHT	Surface Density To Brightness Ratio
PHOT_SPHOT	Spectrophotometric quantities (narrow bands)
PHOT_SPHOT_FLUX	Flux measured (in physical units) in a narrow-band filter (optical, near-IR or near-UV)
PHOT_SPHOT_CONT-GRAD	Pseudo Continuum Gradient
PHOT_SPHOT_CORR-FACT	Spectrophotometry Correction Factor
PHOT_SPHOT_INDEX	Spectrophotometric Index defined by various combinations of narrow-band fluxes
PHOT_SPHOT_INT-ENERGY	Intrinsic Energy in Narrow Spectral Band
PHOT_SPHOT_MAG	Normalized magnitude in a narrow spectral band
PHOT_STR	Stroemgren Photometric System GCPD#4
PHOT_STR_B	Stroemgren Magnitude b (STR)
PHOT_STR_B-R	Stroemgren Color Index b-r (STR)
PHOT_STR_B-V	Stroemgren Color Index b-v (STR)
PHOT_STR_B-Y	Stroemgren Color Index b-y (STR)
PHOT_STR_C1	Stroemgren Color Index c1 (STR)
PHOT_STR_HBETA	Stroemgren Beta Value
PHOT_STR_M1	Stroemgren Color Index m1 (STR)
PHOT_STR_U	Stroemgren Magnitude u (STR)
PHOT_STR_U-B	Stroemgren Color Index u-b (STR)
PHOT_STR_U-V	Stroemgren Color Index u-v (STR)
PHOT_STR_V	Stroemgren Magnitude v (STR)
PHOT_STR_V-B	Stroemgren Color Index v-b (STR)
PHOT_STR_V-Y	Stroemgren Color Index v-y (STR)
PHOT_STR_Y	Stroemgren Magnitude y (STR)
PHOT_SYS-ID	Identification of the Photometric System in use
PHOT_TOT-BRIGHT/B-BRIGHT	Total blue magnitude to Brightness ratio
PHOT_TYCHO	Tycho Photometric System
PHOT_TYCHO_B	Tycho Magnitude B_T_
PHOT_TYCHO_V	Tycho Magnitude V_T_
PHOT_UBVR20	UBVr20 Photometric System GCPD#69
PHOT_UBVR20_B-V20	Color Index B-V20 (UBVr20)
PHOT_UBVR20_U-B20	Color Index U-B20 (UBVr20)
PHOT_UBVR20_V-R20	Color Index V-r20 (UBVr20)
PHOT_UV	UV Magnitude Photometry number # <= Lambda_central < #+100
PHOT_UV_1300	Far UV Magnitude 1300 to 1400 Angstrom UV
PHOT_UV_1400	Far UV Magnitude 1400 to 1500 Angstrom UV
PHOT_UV_1500	Far UV Magnitude 1500 to 1600 Angstrom UV
PHOT_UV_1600	Far UV Magnitude 1600 to 1700 Angstrom UV
PHOT_UV_1700	UV Magnitude 1700 to 1800 Angstrom UV
PHOT_UV_1800	UV Magnitude 1800 to 1900 Angstrom UV
PHOT_UV_1900	UV Magnitude 1900 to 2000 Angstrom UV
PHOT_UV_2000	UV Magnitude 2000 to 2100 Angstrom UV
PHOT_UV_2200	UV Magnitude 2200 to 2300 Angstrom UV
PHOT_UV_2300	UV Magnitude 2300 to 2400 Angstrom UV
PHOT_UV_2400	Near UV Magnitude 2400 to 2500 Angstrom UV
PHOT_UV_2500	Near UV Magnitude 2500 to 2600 Angstrom UV
PHOT_UV_2700	Near UV Magnitude 2700 to 2800 Angstrom UV
PHOT_UV_2945	Near UV Magnitude 2900 to 3000 Angstrom UV
PHOT_UV_3150	Near UV Magnitude 3100 to 3200 Angstrom UV
PHOT_UV_3300	Near UV Magnitude 3300 to 3400 Angstrom UV
PHOT_UV_4250	Near UV Magnitude 4200 to 4300 Angstrom UV
PHOT_UV_COLOR	Ultraviolet Color Index (no bands specified)
PHOT_UV_GENERAL	UV Magnitude unspecified band
PHOT_UVBGRI	UVBGRI Photometric System GCPD#6
PHOT_UVBGRI_B	Filter Blue Magnitude UVBGRI
PHOT_UVBGRI_G	Filter Green Magnitude UVBGRI
PHOT_UVBGRI_I	Filter Infra Magnitude UVBGRI
PHOT_UVBGRI_R	Filter Red Magnitude UVBGRI
PHOT_UVBGRI_U	Filter Ultra Magnitude UVBGRI
PHOT_UVBGRI_V	Filter Violet Magnitude UVBGRI
PHOT_VIL	Vilnius Photometric System GCPD#21
PHOT_VIL_P-X	Vilnius Color Index p-x (VIL)
PHOT_VIL_S-V	Vilnius Color Index s-v (VIL)
PHOT_VIL_U-P	Vilnius Color Index u-p (VIL)
PHOT_VIL_U-V	Vilnius Color Index u-v (VIL)
PHOT_VIL_V	Magnitude V Vilnius (VIL)
PHOT_VIL_V-P	Vilnius Color Index v-p (VIL)
PHOT_VIL_V-S	Vilnius Color Index v-s (VIL)
PHOT_VIL_V-W	Vilnius Color Index v-w
PHOT_VIL_V-X	Vilnius Color Index v-x (VIL)
PHOT_VIL_V-Z	Vilnius Color Index v-z (VIL)
PHOT_VIL_X	Magnitude X Vilnius (VIL)
PHOT_VIL_X-Y	Vilnius Color Index x-y (VIL)
PHOT_VIL_Y-Z	Vilnius Color Index y-z (VIL)
PHOT_VIL_Z-V	Vilnius Color Index z-v (VIL)
PHOT_WASH	Washington Photometric System GCPD#48
PHOT_WASH_C-M	Washington Color Index c-m (WASH)
PHOT_WASH_C-T1	Washington Color Index c-t1 (WASH)
PHOT_WASH_D	Washington Abundance Indicator D (WASH)
PHOT_WASH_M-T1	Washington Color Index m-t1 (WASH)
PHOT_WASH_M-T2	Washington Color Index m-t2 (WASH)
PHOT_WASH_T1	Washington Magnitude t1 (WASH)
PHOT_WLRV	Walraven Photometric System GCPD#11
PHOT_WLRV_B	Walraven Magnitude (flux intensity) B (WLRV)
PHOT_WLRV_B-L	Walraven Color Index B-L (WLRV)
PHOT_WLRV_B-U	Walraven Color Index B-U (WLRV)
PHOT_WLRV_B-W	Walraven Color Index B-W (WLRV)
PHOT_WLRV_L	Walraven Magnitude (Flux Intensity) L (WLRV)
PHOT_WLRV_U	Walraven Magnitude (Flux Intensity) U (WLRV)
PHOT_WLRV_U-W	Walraven Color Index U-W (WLRV)
PHOT_WLRV_V	Walraven Magnitude (Flux Intensity) V (WLRV)
PHOT_WLRV_V-B	Walraven Color Index V-B (WLRV)
PHOT_WLRV_W	Walraven Magnitude (Flux Intensity) W (WLRV)
PHOT_ZP	Zero point coefficient for the photometric system
PHYS	Physical Quantities
PHYS_ABUND	Abundances
PHYS_ABUND_MISC	Abundance (other than H, He, and Fe)
PHYS_ABUND_X	Hydrogen Abundance (X)
PHYS_ABUND_Y	Helium Abundance (Y)
PHYS_ABUND_Z	Metal Abundance Z (metallicity)
PHYS_ABUND_[FE/H]	Fe to H Abundance (Metallicity)
PHYS_ALBEDO	Albedo
PHYS_ANG-MOMENTUM	Angular Momentum
PHYS_AREA	Physical quantities related to Area
PHYS_AREA_CR-SECT	Cross Section
PHYS_AREA_GENERAL	Area (in general)
PHYS_AXIS-RATIO	Axis Ratio
PHYS_BRIGHT	Object's brightness quantities
PHYS_BRIGHT_CHANGE	Brightness Change
PHYS_COLUMN	Line Of Sight Column Properties
PHYS_COLUMN_DENSITY	Column Density (by number of particles)
PHYS_COLUMN_MASS-DENSITY	Mass Column Density
PHYS_COMPACTNESS	Compactness Indicator
PHYS_CONCENT	Concentration Indicators
PHYS_CONCENT_INDEX	Concentration Index
PHYS_DENSITY	Density (various flavours)
PHYS_DENSITY_ELECT	Electron Density
PHYS_DENSITY_ENERGY	Energy Density
PHYS_DENSITY_MASS	Mass Density
PHYS_DENSITY_MASS_SURF	Surface Mass-Density
PHYS_DENSITY_MASS_VOL	Volume Mass-Density
PHYS_DENSITY_NUMBER	Number Density
PHYS_DENSITY_RATIO	Density Ratio
PHYS_DENSITY_SURFACE	Surface Density
PHYS_DISP-MEASURE	Dispersion Measure
PHYS_DISTANCE	Distance and related quantities
PHYS_DISTANCE_DIFF	Distance Difference
PHYS_DISTANCE_NORM	Relative or Normalized Distance
PHYS_DISTANCE_PROJ	Projected Distance
PHYS_DISTANCE_RATIO	Distance Fraction or Ratio
PHYS_DISTANCE_RELATIVE	Relative Distance
PHYS_DISTANCE_TRUE	Distance (true, linear distance)
PHYS_ECCENTRICITY	Eccentricity
PHYS_ELLIPTICITY	Ellipticity
PHYS_EM-MEASURE	Emission Measure
PHYS_ENERGY	Energy and related quantities
PHYS_ENERGY_CONTRIB	Energy Contribution
PHYS_ENERGY_GENERAL	Energy in general
PHYS_ENERGY_INDEX	Energy Index
PHYS_ENERGY_ION	Ion Energy
PHYS_ENERGY_LOSS-RATE	Energy Loss Rate
PHYS_ENERGY_X	X-ray or Gamma-ray Energy
PHYS_EXCITATION	Excitation in the Context of Ionizing Photons
PHYS_EXCITATION_PARAM	Excitation Parameter
PHYS_FLOW	Matter Flow or Outflows Quantities
PHYS_FLOW_POLARITY	Flow Polarity
PHYS_GRADIENT	Gradients (usually on galaxy context)
PHYS_GRADIENT_CHEMICAL	Chemical Gradient
PHYS_GRADIENT_CI	Color Index Gradient
PHYS_GRADIENT_GENERAL	General gradients (usually on galaxy context)
PHYS_GRADIENT_SB	Surface Brightness Gradient
PHYS_GRADIENT_TEMP	Temperature Gradient
PHYS_GRADIENT_VELOCITY	Velocity Gradient
PHYS_GRAVITY	Gravity and related properties
PHYS_GRAVITY_POTENTIAL	Gravitational Potential
PHYS_GRAVITY_PRESS	Gravitational pressure
PHYS_GRAVITY_SURFACE	Surface Gravity
PHYS_HEIGHT	Height or depth (usually in an atmospheric context)
PHYS_IMPACT-PAR	Impact Parameter
PHYS_INV-COMPTON-BEAM-FACT	Inverse Compton Effect Beam Factor
PHYS_IONIZATION	Ionization quantities (in stellar/interstellar environments)
PHYS_IONIZATION_PARAM	Ionization Parameter
PHYS_IONIZATION_PHOTONS	Ionizing Photons
PHYS_IONIZATION_PHOTONS_RATIO	Ionizing Photon Ratio
PHYS_IONIZATION_PHOTONS_TOTAL	Total ionizing Photons
PHYS_LENGTH	Length related quantities
PHYS_LENGTH_RATIO	Length Ratio
PHYS_LIMB-DARK	Limb Darkening Phenomena
PHYS_LIMB-DARK_COEFF	Limb Darkening Coefficient
PHYS_LUMINOSITY	Luminosity, in different bands and types
PHYS_LUMINOSITY_B	Luminosity in blue light
PHYS_LUMINOSITY_CARBON	Carbon luminosity
PHYS_LUMINOSITY_CONTINUUM	Continuum luminosity
PHYS_LUMINOSITY_DENSITY	Luminosity density
PHYS_LUMINOSITY_R	Luminosity in red light
PHYS_LUMINOSITY_GENERAL	Luminosity in general
PHYS_LUMINOSITY_H2O	Water maser luminosity
PHYS_LUMINOSITY_HALPHA	H alpha luminosity
PHYS_LUMINOSITY_HBETA	H beta luminosity
PHYS_LUMINOSITY_HE	Helium luminosity
PHYS_LUMINOSITY_HYDROG	Hydrogen luminosity
PHYS_LUMINOSITY_IR	Infrared luminosity
PHYS_LUMINOSITY_IR_100	Luminosity at 100 micron
PHYS_LUMINOSITY_IR_12	Luminosity at 12 micron
PHYS_LUMINOSITY_IR_25	Luminosity at 25 micron
PHYS_LUMINOSITY_IR_60	Luminosity at 60 micron
PHYS_LUMINOSITY_IR_MISC	Infrared luminosity in general
PHYS_LUMINOSITY_MASER	Maser luminosity
PHYS_LUMINOSITY_NU	Neutrino luminosity
PHYS_LUMINOSITY_OH	OH luminosity
PHYS_LUMINOSITY_PROFILE	Luminosity profile
PHYS_LUMINOSITY_RADIO	Radio luminosity
PHYS_LUMINOSITY_RATIO	Luminosity ratio
PHYS_LUMINOSITY_SURFACE	Surface luminosity
PHYS_LUMINOSITY_UV	Ultraviolet luminosity
PHYS_LUMINOSITY_UV_LYA	Ionizing ultraviolet luminosity in lyman alpha
PHYS_LUMINOSITY_UV_MISC	Ultraviolet luminosity
PHYS_LUMINOSITY_X	X-ray luminosity
PHYS_MAG-FIELD	Magnetic Field
PHYS_MASS	Mass and related quantities
PHYS_MASS_ABS-COEFF	Mass Absorption Coefficient
PHYS_MASS_FUNCTION	Function of mass, typically in spectroscopic binaries (M2*sini)^3^/(M1+M2)^2^
PHYS_MASS_FLUX	Mass flux or flow
PHYS_MASS_FRACTIONAL	Fractional Mass
PHYS_MASS_LOSS	Mass Loss
PHYS_MASS_MISC	Mass
PHYS_MASS_RATIO	Mass Ratio
PHYS_MASS_YIELD	Mass yield associated to a given element
PHYS_MASS/LIGHT	Mass to Light Ratio
PHYS_OPACITY	Opacity
PHYS_OPTICAL-DEPTH	Optical Depth
PHYS_OUTFLOW	Outflows related quantities
PHYS_OUTFLOW_PARAM	Outflow Parameter Factor
PHYS_PLASMA_PARAM	Plasma Physics Parameters
PHYS_PLASMA_GAUNT-FACT	Plasma Physics Gaunt Factor
PHYS_PRESS	Pressure and related quantities
PHYS_PRESS_ELECT	Electron Pressure
PHYS_PRESS_GAS	Gas Pressure
PHYS_RAD-MAX-ROT-VEL	Radius at which maximum rotational velocity occurs
PHYS_RADIATIVE-ACCEL	Radiative Acceleration
PHYS_REFLECTANCE	Reflectance
PHYS_REFRACT-INDX	Refraction Index
PHYS_ROTATION-MEASURE	Rotation Measure
PHYS_SCALE	Quantities Representing a Scale
PHYS_SCALE_HEIGHT	Scale Height
PHYS_SCALE_LENGTH	Scale Length
PHYS_SEPARATION	Pair Separation (in non-angular units)
PHYS_SIZE	Size (in non-angular units)
PHYS_SIZE_DIAM	Diameter
PHYS_SIZE_MAJ	Size (diameter) measured along the major axis
PHYS_SIZE_MIN	Size (diameter) measured along the minor axis
PHYS_SIZE_RADIUS	Radius and related quantities
PHYS_SIZE_RADIUS_GENERAL	Linear Radius
PHYS_SIZE_RADIUS_NORM	Normalized Radius
PHYS_SIZE_RATIO	Size Ratio
PHYS_SIZE_SMAJ	Size Of The Semi Major Axis
PHYS_SIZE_SMAJ_GENERAL	Size Of The Semi Major Axis
PHYS_SIZE_SMAJ_NORM	Normalized Size of the Major Axis
PHYS_SIZE_SMIN	Size of the Semi Minor Axis
PHYS_SIZE_SMIN_NORM	Normalized Size of the Minor Axis
PHYS_STAR-FORM	Star Formation Related Quantities
PHYS_STAR-FORM_RATE	Star Formation Rate
PHYS_SUN	Solar Related Quantities
PHYS_SUN_ATM	Quantities Related to the Solar Atmosphere
PHYS_SUN_ATM_ABS-COEFF	Solar Spectral Absorption Coefficient
PHYS_SUN_ATM_PARAM	Solar Atmosphere Parameter
PHYS_SUN_HARM/FUN-BAND-FREQ-RATIO	Harmonic to Fundamental Frequency Ratio
PHYS_TANG-DOPPLER-FACT	Tangential Doppler Effect Factor
PHYS_TEMP	Temperature and related quantities
PHYS_TEMP_DIFF	Temperature Amplitude or difference
PHYS_TEMP_EFFEC	Effective Temperature
PHYS_TEMP_ELECT	Electron Temperature
PHYS_TEMP_EXCIT	Excitation Temperature
PHYS_TEMP_F-F	Free-free or Bremsstrahlung Temperature
PHYS_TEMP_KINETIC	Kinetic Temperature
PHYS_TEMP_MISC	Temperature in general
PHYS_TEMP_PLASMA	Plasma Temperature
PHYS_TEMP_THETA	Effective temperature theta (5040/Teff)
PHYS_TEMP_XRAY	X Ray temperature
PHYS_TYPE	Type of Phenomenon or Event
PHYS_VOLUME	Volume
PHYS_VOLUME_RATIO	Volume Ratio
PHYS_WIND	Stellar or Solar Wind Properties
PHYS_WIND_LUMINOSITY	Wind Luminosity
POL	Polarization Related Quantities
POL_DEGREE	Degree of Polarization
POL_DEGREE_CIRC	Degree of Circular polarization
POL_DEGREE_LINEAR	Degree of Linear polarisation
POL_DEGREE_MISC	Degree of Polarization (unspecified type)
POL_FLUX	Polarized Flux (two flavours)
POL_FLUX_LCP	Left Circular Polarization Flux
POL_FLUX_LINEAR	Linear polarized flux density
POL_FLUX_RCP	Right Circular Polarization Flux
POL_INDEX	Polarization Index
POL_LAMBDA-MAX	Maximum Polarization's Wavelength
POL_LINEAR/CIRC	Ratio of Linear to Circular Polarization
POL_PA	A vector's Position Angle
POL_PA_EQ	Position Angle in Equatorial Coordinates
POL_PA_GAL	Position Angle in Galactic Coordinates
POL_PA_MISC	Vector's Position Angle in unspecified coordinate system
POL_STOKES_Q	Stokes parameter Q (absolute, or relative Q/I) [horizontal/vertical component]
POL_STOKES_I	Stokes parameter I (total power)
POL_SENSE	Sense of (circular) Polarization
POL_SLOPE	Polarimetry Slope
POL_STOKES_U	Stokes parameter U (absolute, or relative U/I) [diagonal component]
POL_STOKES	Reduced Stokes Parameter U
POL_STOKES_V	Stokes parameter V (absolute, or relative V/I) [circular component]
POS	Position Related Quantities
POS_ANG	Angular Position
POS_ANG_DIST	Angular Distance and related quantities
POS_ANG_DIST_GENERAL	Angular Distance Or Separation
POS_ANG_DIST_REL	Relative Angular Distance
POS_ANG_DIST_SQ	Quadratic Angular Distance
POS_ANG_VEL	Rate Of Position Change (drift motion, angular velocity)
POS_CCD	Positions Related To CCD's
POS_CCD_X	CCD Position Along the X Axis
POS_CCD_Y	CCD Position Along the Y Axis
POS_DETECTOR	Position Related to the Detector
POS_DETECTOR_DIST	Distance Or Position In Detector Units
POS_DETECTOR_RADIUS	Radius of an Object Expressed In Detector's Unit
POS_DIR-COSINE	Direction Cosine
POS_EARTH	Positions On The Earth
POS_EARTH_LAT	Earth's Latitude
POS_EARTH_LAT_MAIN	Earth's Latitude
POS_EARTH_LAT_VAR	Variation of Local Latitude
POS_EARTH_LOCATION	Earth Location
POS_EARTH_LON	Earth Longitude
POS_EC	Ecliptic Coordinates and derivates
POS_EC_LAT	Ecliptic Latitude
POS_EC_LON	Ecliptic Longitude
POS_EQ	Equatorial Coordinates and related quantities
POS_EQ_A-V-PRECESS	Annual Variation of Precession in RA
POS_EQ_DEC	Declination related quantities
POS_EQ_DEC_3T	Third Term in Declination
POS_EQ_DEC_MAIN	Declination
POS_EQ_DEC_OFF	Declination Offset Difference
POS_EQ_DEC_OTHER	Declination in Non-Standard Units or partial values
POS_EQ_DEC_PRECESS	Precession Variation in Declination
POS_EQ_DEC_REL	Relative Declination in a Special Scale
POS_EQ_PLX	Relations between Parallax and RA and Dec
POS_EQ_PLX_FACTOR	Parallax Factor in Declination
POS_EQ_PM	Total proper motion (can be in non-equatorial frame)
POS_EQ_PMRA	Proper Motion in Right Ascension (pmra)
POS_EQ_PMDEC	Proper Motion in Declination (pmdec)
POS_EQ_PM-PA	Position angle (North through East) of Proper Motion vector
POS_EQ_X	X component of equatorial position: x=cos(Dec)cos(RA)
POS_EQ_Y	Y component of equatorial position: y=cos(Dec)sin(RA)
POS_EQ_Z	Z component of equatorial position: z=sin(Dec)
POS_EQ_PREC	Annual Precession Quantities
POS_EQ_PREC_DEC	Annual Precession In Declination
POS_EQ_PREC_RA	Precession Variation In RA
POS_EQ_RA	Right Ascension related quantities
POS_EQ_RA_2T	Second Component in right Ascension
POS_EQ_RA_3T	Third Term In Right Ascension
POS_EQ_RA_CORR	Correction in Right Ascension
POS_EQ_RA_MAIN	Right Ascension
POS_EQ_RA_OFF	RA Offset or Residual In Right Ascension
POS_EQ_RA_OTHER	Right Ascension in Non-Standard Units or partial values
POS_EQ_RA_REL	Relative Right Ascension in a Special Scale
POS_GAL	Galactic Coordinates and related quantities
POS_GAL_COSEC-B	Cosecant of galactic latitude
POS_GAL_LAT	Galactic Latitude
POS_GAL_LON	Galactic Longitude
POS_GAL_GC	Galactocentric Distance
POS_GENERAL	Position in general
POS_GEO	Geocentric Quantities
POS_GEO_ANGLE	Angle Of The Geocenter
POS_GEO_DEC	Geocentric declination
POS_GEO_RA	Geocentric Right Ascension
POS_HA	Hour Angle
POS_HC_X	Heliocentric X
POS_HC_Y	Heliocentric Y
POS_HC_Z	Heliocentric Z
POS_INCLIN	Inclination angles
POS_INCLIN_EC	Inclination Respect to the ecliptic
POS_INCLIN_GP	Inclination Respect to the Galactic Plane
POS_INCLIN_LOS	Inclination Respect to the Line Of Sight
POS_JOVIC	Jovicentric Coordinates (Jupiter's Phenomena)
POS_JOVIC_X	Jovicentric X
POS_JOVIC_Y	Jovicentric Y
POS_GAL_HC	Heliocentric Distance
POS_GAL_X	X coordinate of object in Galactic Plane: x=r.cos(GLAT)cos(GLON)
POS_GAL_Y	Y coordinate of object in Galactic Plane: y=r.cos(GLAT)sin(GLON)
POS_GAL_Z	Z coordinate of object above Galactic Plane: z=r.sin(GLAT)
POS_LIMIT	Position Limit to an Observation
POS_LITERAL	Literal Alpha-Delta Identification of a Position
POS_LOCATION	Location of certain events not easily expressed in other categories
POS_MAP	Quantity Measurement on a Contour Map
POS_OCCULT	Quantity related to the lunar occultations
POS_OCCULT_DIR	Direction of lunar motion
POS_OCCULT_POS	Quantity related to the lunar occultations
POS_OCCULT_SLOPE	Lunar Slope
POS_OFFSET	Positional offsets, usually a string
POS_PAR-ANG	Parallactic Angle
POS_PARLX	Parallax and related quantities
POS_PARLX_DYN	Dynamical Parallax
POS_PARLX_PHOT	Photometric Parallax
POS_PARLX_RADIO	Radio Parallax
POS_PARLX_SPEC	Spectroscopic Parallax
POS_PARLX_TRIG	Trigonometric Parallax
POS_PLANETARY	Coordinates in a System Related Non-Jovian Planets
POS_PLATE	Positions measured in photographic plates
POS_PLATE_DIFF	Difference in position or separation between objects
POS_PLATE_X	X Coordinate on a Plate
POS_PLATE_Y	Y Coordinate on a Plate
POS_PM	Proper Motion (non-equatorial) and related quantities
POS_PM_DIFF	Difference In Proper Motion
POS_PM_NON-EQ	Proper Motion (non-equatorial)
POS_PM_PA	Polar Angle of Proper Motion Vector in a non-equatorial frame
POS_POS-ANG	Position Angle (PA) of a certain vector
POS_PRECESSION	Precession
POS_RADIUS	Radius Used To Calculate Other Quantity
POS_REFERENCE-SYSTEM	Used Reference System
POS_SG	Super Galactic Coordinates
POS_SG_LAT	Supergalactic Latitude
POS_SG_LON	Supergalactic Longitude
POS_SG_X	Supergalactic X coordinate
POS_SG_Y	Supergalactic Y coordinate
POS_SG_Z	Supergalactic Z coordinate
POS_SOLAR	Solar Positions
POS_SOLAR_ELEVAT	Solar Elevation
POS_SOLAR_ELONG	Solar Elongation
POS_TANG-PLANE	Tangent Plane Position or a system attached to an object
POS_TOPO	Topocentric Positions
POS_TOPO_DEC	Topocentric Declination
POS_TOPO_RA	Topocentric right ascension
POS_VAR	Positional Variations
POS_VAR_RATE	Rate of Variation of positional quantities
POS_ZD	Zenith Distance and related quantities
POS_ZD_MAIN	Zenith Distance
POS_ZD_RES	Residual In Zenith Distance
RECORD	Record Number
REDSHIFT	Redshift
REDSHIFT_DIFF	Difference in redshift (usually between companions or nearby objects)
REDSHIFT_GC	Galactocentric Redshift
REDSHIFT_HC	Redshift (normally heliocentric)
REDUCT	Quantities Associated with the Reduction Process
REDUCT_EXTR-RAD	Extraction Radius
REDUCT_METHOD	Reduction Method or Technique
REDUCT_PARAM	Reduction Parameter
REFER	References
REFER_BIBCODE	Reference Bibliographic Code
REFER_CODE	References (or reference code)
REFER_TEXT	Text related to a reference, may include author, journal, editor, publisher,...
REFER_JOURN	Journal/Publication
REFER_PAGE	Page Number
REFER_VOL	Volume Number or Identification
REMARKS	Remark or Comments
SPECT	Spectroscopy and related quantities
SPECT_BALMER	Properties of hydrogen balmer series
SPECT_BALMER_DEC	Balmer Decrement
SPECT_BALMER_JUMP	Balmer Jump
SPECT_CONTINUUM	Continuum Properties
SPECT_CONTINUUM_CORR-FACT	Continuum Correction Factor
SPECT_CONTINUUM_DEPTH	Continuum Depth
SPECT_CONTINUUM_INDICATOR	Continuum Indicator
SPECT_CONTINUUM_PROP	Continuum Properties
SPECT_DOPPLER-PAR	Doppler Parameter
SPECT_EMISSIVITY	Emissivity In A Certain Waveband
SPECT_EQ-WIDTH	Equivalent Width
SPECT_FEATURE	Spectroscopic Feature properties
SPECT_FEATURE_PROP	Spectroscopic Feature properties
SPECT_FEATURE_WIDTH	Equivalent Width of a given Feature
SPECT_FLUX	Flux, usually in a narrow spectral band
SPECT_FLUX_NORM	Normalized Flux, usually in a narrow spectral band
SPECT_FLUX_RATIO	Spectroscopic flux ratio
SPECT_FLUX_UV	Spectroscopy line flux in the uv
SPECT_FLUX_VALUE	Flux, usually in a narrow spectral band
SPECT_GENERAL	Spectroscopy in general
SPECT_HARDNESS-RATIO	Hardness ratio usually in X-ray
SPECT_ID	Spectral identification
SPECT_INDEX	Spectroscopic index
SPECT_INDEX_BANDPASS	Spectroscopic index bandpass
SPECT_INDEX_HBETA	H Beta spectroscopic index
SPECT_INDEX_MISC	Miscellaneous spectroscopic index
SPECT_INTEGRAL	Integral spectrum
SPECT_INTENSITY	Spectral Intensity
SPECT_INTENSITY_ESTIMATED	Estimated Intensity
SPECT_INTENSITY_FR-DROP	Intensity Drop Fraction
SPECT_INTENSITY_HBETA-NORM	Hbeta Normalized Intensity
SPECT_INTENSITY_INST-UNIT	Intensity In Instrumental Units
SPECT_INTENSITY_MAIN	Spectral Intensity
SPECT_INTENSITY_RATIO	Intensity Ratio
SPECT_INTENSITY_REL	Relative Intensity
SPECT_LINE	Spectral Line Properties
SPECT_LINE_BROADENING	Line Broadening
SPECT_LINE_CENT	Line Central Position
SPECT_LINE_DEPTH	Line Depth
SPECT_LINE_DEPTH_DIFF	Difference In Line Depth
SPECT_LINE_DEPTH_VALUE	Line Depth
SPECT_LINE_ENERGY	Line Energy
SPECT_LINE_FREQUENCY	Line Frequency (usually in radio)
SPECT_LINE_FWHM	Line Full Width Half Maximum (FWHM)
SPECT_LINE_ID	Line Identification
SPECT_LINE_INTENSITY	Line Intensity
SPECT_LINE_MOMENT	Line Moment
SPECT_LINE_RATIO	Line Ratio
SPECT_LINE_STRENGTH	Line Strength
SPECT_LINE_TEMP	Line temperature
SPECT_LINE_WIDTH	Line Width
SPECT_LUM-CLASS	Luminosity Classification
SPECT_LUM/WVLNGTH-INT	Luminosity per Wavelength Interval
SPECT_LUMINOSITY	Monochromatic Luminosity
SPECT_NORMALIZED	Normalized Spectrum
SPECT_PECUL	Spectral Peculiarities
SPECT_POWER	Spectral Power
SPECT_RANGE	Spectral Range
SPECT_RESOLUTION	Spectral Resolution
SPECT_S/N	Spectrum Signal To Noise Ratio
SPECT_SENSITIVITY	Spectral sensitivity
SPECT_SOFTNESS-RATIO	Softness ratio usual in x ray
SPECT_SP+INDEX	Spectral Index = d(Log F)/d(Log nu)
SPECT_SP-INDEX	Spectral Index = -d(Log F)/d(Log nu)
SPECT_STARK	Stark effect related quantities
SPECT_SUN	Solar Spectrum
SPECT_TYPE	Spectrum Classification
SPECT_TYPE_GENERAL	Spectrum Classification
SPECT_TYPE_MK	MK Spectral Classification
SPECT_TYPE_RADIO	Radio Spectral Type
SPECT_VELOC	Velocity (associated with lines)
SPECT_VELOC_VALUE	Velocity (associated with lines)
SPECT_VELOC_WIDTH	Velocity width
SPECT_WAVELENGTH	Wavelength (associated to lines)
SPECT_WAVELENGTH_CENTRAL	Central wavelength
SPECT_WAVELENGTH_DIFF	Difference in Wavelength
SPECT_WAVELENGTH_MISC	Wavelength (associated to lines)
STAT	Statistical Properties
STAT_%REJECT	Percent of Rejection
STAT_COMPLETENESS	Degree of Completeness of a Sample
STAT_CORRELATION	Correlation
STAT_LIKELIHOOD	Maximum Likelihood of existence or occurance
STAT_LIKELIHOOD-RATIO	Likelihood Ratio
STAT_MEAN	Statistics Mean Value
STAT_MEDIAN	Statistics Median Value
STAT_N-DOF	Degrees of Freedom
STAT_PARAM	Statistic Parameter or Factor
STAT_PROBABILITY	Probability
STAT_PROP	Statistical Properties
STAT_SAMP-FACTOR	Sampling Factor
STAT_SIGNIFICANCE	Statistical Significance
TEL	Telescopes
TEL_SIZE	Telescope size (dimension)
TEL_FOCAL-LENGTH	Focal Length
TEL_ID	Telescope Identification
TIME	Time and related Quantities
TIME_AGE	Age
TIME_CROSSING	Crossing Time
TIME_CYCLE	Cycle number of a variable object.
TIME_DATE	Date (Julian Date or Heliocentric Julian date)
TIME_DELAY	Time Delay
TIME_DIFF	Time Difference O-C Residual
TIME_DP/DT	Period Rate Of Change
TIME_EPOCH	Epoch
TIME_EQUINOX	Equinox
TIME_EVOLUTION	Evolution Time
TIME_EXPTIME	Exposure Time
TIME_INTERVAL	Time Interval
TIME_LIMIT	Time Limit
TIME_MISC	Time in general
TIME_PERIOD	Period
TIME_PHASE	Phase (in the context of periodic variable objects)
TIME_RATE	Rate Of Certain Phenomenon
TIME_RELAXATION	Relaxation Time
TIME_RESOLUTION	Time resolution
TIME_SCALE	Time Scale
TIME_ZONE	Time Zone
UNITS	Units in which a quantity is measurement
VAR	Quantities related to variable objects
VAR_AMPLITUDE	Amplitude of variation and related quantities
VAR_AMPLITUDE_RATIO	Amplitude Ratio
VAR_AMPLITUDE_VALUE	Amplitude of variation
VAR_CLASS	Type of variability
VAR_DF/DT2	2nd time derivative of barycentric rotation frequency in seconds
VAR_DF/DT3	3rd time derivative of barycentric rotation frequency in seconds
VAR_ECL-CYC-N	Eclipse Cycle Number
VAR_FRACT-LIGHT	Fraction Light
VAR_INDEX	Variability Index
VAR_LIGHT-DROP	Light Drop
VAR_MAG-RANGE	Magnitude Range
VAR_MEAN	Quantity at stage of mean
VAR_MODEL-FIT	Variability Fit Parameter
VAR_PERIOD	Period of Variability and related quantities
VAR_PERIOD_VAR	Period Variations
VAR_PRIM-MIN	Primary Minimum Importance
VAR_PROBABILITY	Probability of Variability
VAR_PULSE	Quantities related to pulses (pulsars)
VAR_PULSE_EQ-WIDTH	Pulse Equivalent Width
VAR_PULSE_WIDTH	Pulse Width
VAR_RAD-OSCILL	Radial Oscillation Parameter
VAR_RRLYRA-FREQ	Frequency Of RR Lyrae
VAR_SEC-MIN	Secondary Minimum Importance
VELOC	Velocity
VELOC_BARYCENTER	Barycenter Velocity
VELOC_CM	Velocity Refered to a Co-Moving System
VELOC_CM_X	Comoving Velocity Along X Eastward
VELOC_CM_Y	Comoving Velocity Along Y Northward
VELOC_CM_Z	Comoving Velocity Along the Line of Sight
VELOC_CMB	Radial Velocity respect to the 3k CMB
VELOC_CORR	Velocity Correction
VELOC_DIFF	Velocity Difference
VELOC_DISP	Velocity Dispersion
VELOC_ESCAPE	Escape Velocity
VELOC_EXPANSION	Expansion Velocity
VELOC_GAL	Space Velocity In Galactic Coordinates
VELOC_GAL_PHI	Space Velocity In Galactic Coordinate Phi Component
VELOC_GAL_RHO	Space Velocity In Galactic Coordinate Rho Component
VELOC_GAL_U	Space Velocity In Galactic Coordinate U Component
VELOC_GAL_V	Space Velocity In Galactic Coordinate V Component
VELOC_GAL_W	Space Velocity In Galactic Coordinate W Component
VELOC_GC	Galactocentric Radial Velocity
VELOC_GEOC	Geocentric Radial Velocity
VELOC_HC	Heliocentric Radial Velocity
VELOC_LG	Local Group Radial Velocity
VELOC_LSR	Radial Velocity Respect to the Local Standard of Rest
VELOC_MAX	Maximum or Terminal Velocity
VELOC_MEAN	Mean Velocity
VELOC_MICRO-TURB	Microturbulence Velocity
VELOC_MISC	Velocity in general
VELOC_OBS	Observed velocity (without corrections)
VELOC_OCCULT	Occultation Velocity
VELOC_ORBIT	Orbital Velocity
VELOC_PECULIAR	Peculiar Velocity
VELOC_PRE-ENTRY	Pre-Entry Velocity (meteorites)
VELOC_PULSAT	Pulsation Velocity
VELOC_RANGE	Velocity Range
VELOC_RELAT	Relative Velocity
VELOC_RESID	Residual velocity (any component or system)
VELOC_RMS	Velocity RMS
VELOC_ROTAT	Rotational Velocity
VELOC_SPACE	Space Velocity
VELOC_SPACE_X	Space Velocity X Component
VELOC_SPACE_Y	Space Velocity Y Component
VELOC_SPACE_Z	Space Velocity Z Component
VELOC_SYST	Systemic Velocity
VELOC_SYST_HC	Heliocentric Systemic Velocity
VELOC_SYST_MISC	Systemic Velocity
VELOC_TANG	Tangential Velocities
VELOC_TANG_GAL	Tangential Velocity in Galactic Frame
VELOC_TANG_MISC	Tangential Velocity
VELOC_TANG_PEC	Peculiar Tangential Velocity
VELOC_TOTAL	Total Velocity
VELOC_WIND	Wind Velocity
WEIGHT	Statisctical Weight Associated to Data Fits
PHYS_ELEC-FIELD	Electric (electrostatic) Field
PHOT_FLUX_IR_6	Flux density around 6 microns (e.g. ISO at 6.7 microns)
POS_PM_DISP	Dispersion in proper motions (typically in clusters)
SPECT_INDEX_HALPHA	Spectroscopic index H{alpha}
SPECT_INDEX_HGAMMA	Spectroscopic index H{gamma}
PHOT_SDSS_U	Magnitude in u' filter of Sloan Digital Sky Survey (1996AJ....111.1748F)
PHOT_SDSS_G	Magnitude in g' filter of Sloan Digital Sky Survey (1996AJ....111.1748F)
PHOT_SDSS_R	Magnitude in r' filter of Sloan Digital Sky Survey (1996AJ....111.1748F)
PHOT_SDSS_I	Magnitude in i' filter of Sloan Digital Sky Survey (1996AJ....111.1748F)
PHOT_SDSS_Z	Magnitude in z' filter of Sloan Digital Sky Survey (1996AJ....111.1748F)
PHOT_FLUX_IR_9	Flux density around 9 microns
PHOT_FLUX_IR_170	Far infra-red Flux density around 170um (1750GHz)
PHOT_FLUX_IR_300	Far infra-red Flux density around 300um (3000GHz)
PHOT_TRANSF_PARAM	Parameter used in photometric transformations
POS_TRANSF_PARAM	Parameter used in astrometric transformations, e.g. WCS constants
POS_LAMBERT	Coordinates in the Lambert Projection
POS_LAMBERT_R	Lambert Polar Distance
POS_LAMBERT_X	Lambert X Coordinate
POS_LAMBERT_Y	Lambert Y Coordinate
VELOC_GAL_MISC	Miscellaneous Velocities, like Total or Tangent velocity
STAT_COVAR	Statistical covariance parameter
STAT_STDEV	Statistical standard deviation (square root of the variance)
STAT_VAR	Statistical variance (squared standard deviation)

# UCD 1+ (en lowercase pour les noms des UCD)
arith	Arithmetic quantities
arith.diff	Difference between two quantities described by the same UCD
arith.factor	Numerical factor
arith.grad	Gradient
arith.rate	Rate (per time unit)
arith.ratio	Ratio between two quantities described by the same UCD
arith.zp	Zero point
em	Electromagnetic spectrum
em.ir	Infrared part of the spectrum
em.ir.15-30um	Infrared between 15 and 30 micron
em.ir.3-4um	Infrared between 3 and 4 micron
em.ir.30-60um	Infrared between 30 and 60 micron
em.ir.4-8um	Infrared between 4 and 8 micron
em.ir.60-100um	Infrared between 60 and 100 micron
em.ir.8-15um	Infrared between 8 and 15 micron
em.ir.h	Infrared between 1.5 and 2 micron
em.ir.j	Infrared between 1.0 and 1.5 micron
em.ir.k	Infrared between 2 and 3 micron
em.uv	Ultraviolet part of the spectrum
em.uv.10-50nm	Ultraviolet between 10 and 50 nm
em.uv.100-200nm	Ultraviolet between 100 and 200 nm
em.uv.200-300nm	Ultraviolet between 200 and 300 nm
em.uv.50-100nm	Ultraviolet between 50 and 100 nm
em.x-ray	X-ray part of the spectrum
em.x-ray.hard	Hard X-ray (12 - 120 keV)
em.x-ray.medium	Medium X-ray (2 - 12 keV)
em.x-ray.soft	Soft X-ray (0.12 - 2 keV)
em.energy	Energy value in the em frame
em.freq	Frequency value in the em frame
em.gamma	Gamma rays part of the spectrum
em.gamma.hard	Hard gamma ray (>500 keV)
em.gamma.soft	Soft gamma ray (120 - 500 keV)
em.line	Designation of major atomic lines
em.line.brgamma	Bracket gamma line
em.line.hi	21cm hydrogen line
em.line.halpha	H-alpha line
em.line.hbeta	H-beta line
em.line.hgamma	H-gamma line
em.line.oiii	[OIII] line
em.mm	Millimetric part of the spectrum
em.mm.100-200ghz	Millimetric between 100 and 200 GHz
em.mm.1500-3000ghz	Millimetric between 1500 and 3000 GHz
em.mm.200-400ghz	Millimetric between 200 and 400 GHz
em.mm.30-50ghz	Millimetric between 30 and 50 GHz
em.mm.400-750ghz	Millimetric between 400 and 750 GHz
em.mm.50-100ghz	Millimetric between 50 and 100 GHz
em.mm.750-1500ghz	Millimetric between 750 and 1500 GHz
em.opt	Optical part of the spectrum
em.opt.b	Optical band between 400 and 500 nm
em.opt.i	Optical band between 750 and 1000 nm
em.opt.r	Optical band between 600 and 750 nm
em.opt.u	Optical band between 300 and 400 nm
em.opt.v	Optical band between 500 and 600 nm
em.radio	Radio part of the spectrum
em.radio.100-200mhz	Radio between 100 and 200 MHz
em.radio.12-30ghz	Radio between 12 and 30 GHz
em.radio.1500-3000mhz	Radio between 1500 and 3000 MHz
em.radio.20-100mhz	Radio between 20 and 100 MHz
em.radio.200-400mhz	Radio between 200 and 400 MHz
em.radio.3-6ghz	Radio between 3 and 6 GHz
em.radio.400-750mhz	Radio between 400 and 750 MHz
em.radio.6-12ghz	Radio between 6 and 12 GHz
em.radio.750-1500mhz	Radio between 750 and 1500 MHz
em.wavenumber	Wavenumber value in the em frame
em.wl	Wavelength value in the em frame
em.wl.central	Central wavelength
em.wl.effective	Effective wavelength
instr	Instrument
instr.background	Instrumental background
instr.bandpass	Bandpass (e.g.: band name) of instrument
instr.bandwidth	Bandwidth of the instrument
instr.baseline	Baseline for interferometry
instr.beam	Beam
instr.calib	Calibration parameter
instr.det	Detector
instr.det.noise	Instrument noise
instr.det.psf	Point Spread Function
instr.det.qe	Quantum efficiency
instr.dispersion	Dispersion of a spectrograph
instr.filter	Filter
instr.fov	Field of view
instr.obsty	Observatory, satellite, mission
instr.obsty.seeing	Seeing
instr.offset	Offset angle respect to main direction of observation
instr.order	Spectral order in a spectrograph
instr.param	Various instrumental parameters
instr.pixel	Pixel (default size: angular)
instr.plate	Photographic plate
instr.plate.emulsion	Plate emulsion
instr.precision	Instrument precision
instr.saturation	Instrument saturation threshold
instr.scale	Instrument scale (for CCD, plate, image)
instr.sensitivity	Instrument sensitivity, detection threshold
instr.setup	Instrument configuration or setup
instr.skylevel	Sky level
instr.skytemp	Sky temperature
instr.tel	Telescope
instr.tel.focallength	Telescope focal length
meta	Metadata
meta.bib	Bibliographic reference
meta.bib.author	Author name
meta.bib.bibcode	Bibcode
meta.bib.fig	Figure in a paper
meta.bib.journal	Journal name
meta.bib.page	Page number
meta.bib.volume	Volume number
meta.code	Code or flag
meta.code.class	Classification code
meta.code.error	limit uncertainty error flag
meta.code.member	Membership code
meta.code.mime	MIME type
meta.code.multip	Multiplicity or binarity flag
meta.code.qual	Quality, precision, reliability flag or code
meta.cryptic	Unknown or impossible to understand quantity
meta.curation	Identity of man/organization responsible for the data
meta.dataset	Dataset
meta.file	File
meta.fits	FITS standard
meta.id	Identifier, name or designation
meta.id.assoc	Identifier of associated counterpart
meta.id.cross	Cross identification
meta.id.parent	Identification of parent source
meta.id.part	Part of identifier, suffix or sub-component
meta.main	Main value of something
meta.modelled	Quantity was produced by a model
meta.note	Note or remark (longer than a code or flag)
meta.number	Number (of things; e.g. nb of object in an image)
meta.record	Record number
meta.ref	Reference, or origin
meta.ref.url	URL, web address
meta.software	Software used in generating data
meta.table	Table or catalogue
meta.title	Title or explanation
meta.ucd	UCD
meta.unit	Unit
meta.version	Version
obs	Observation
obs.airmass	Airmass
obs.atmos	Atmosphere
obs.atmos.extinction	Atmospheric extinction
obs.atmos.refractangle	Atmospheric refraction angle
obs.calib	Calibration observation
obs.field	Region covered by the observation
obs.image	Image
obs.observer	Observer, discoverer
obs.param	Various observation or reduction parameter
phot	Photometry
phot.antennatemp	Antenna temperature
phot.calib	Photometric calibration
phot.color	Color index or magnitude difference
phot.color.excess	Color excess
phot.color.reddfree	Dereddened color
phot.count	Flux expressed in counts
phot.fluence	Fluence
phot.flux	Photon flux
phot.flux.bol	Bolometric flux
phot.flux.density	Flux density (per wl/freq/energy interval)
phot.flux.density.sb	Flux density surface brightness
phot.flux.sb	Flux surface brightness
phot.limbdark	Limb-darkening coefficients
phot.mag	Photometric magnitude
phot.mag.bc	Bolometric correction
phot.mag.bol	Bolometric magnitude
phot.mag.distmod	Distance modulus
phot.mag.reddfree	Dereddened magnitude
phot.mag.sb	Surface brightness in magnitude units
phys	Physical quantities
phys.sfr	Star formation rate
phys.absorption	Extinction or absorption along the line of sight
phys.absorption.coeff	Absorption coefficient (e.g. in a spectral line)
phys.absorption.gal	Galactic extinction
phys.absorption.opticaldepth	Optical depth
phys.abund	Abundance
phys.abund.fe	Fe/H abundance
phys.abund.x	Hydrogen abundance
phys.abund.y	Helium abundance
phys.abund.z	Metallicity abundance
phys.acceleration	Acceleration
phys.albedo	Albedo or reflectance
phys.angarea	Angular area
phys.angmomentum	Angular momentum
phys.angsize	Angular size width diameter dimension extension major minor axis extraction radius
phys.angsize.smajaxis	Angular size extent or extension of semi-major axis
phys.angsize.sminaxis	Angular size extent or extension of semi-minor axis
phys.area	Area (in linear units)
phys.atmol	Atomic and molecular physics
phys.atmol.branchingratio	Branching ratio
phys.atmol.collstrength	Collisional strength
phys.atmol.collisional	Related to collisions
phys.atmol.configuration	Configuration
phys.atmol.crosssection	Atomic / molecular cross-section
phys.atmol.damping	Atomic damping quantities (van der Waals)
phys.atmol.element	Element
phys.atmol.excitation	Atomic molecular excitation parameter
phys.atmol.final	Quantity refers to atomic/molecular final/ground state, level, ecc.
phys.atmol.initial	Quantity refers to atomic/molecular initial state, level, ecc.
phys.atmol.ionstage	Ion
phys.atmol.ionization	Related to ionization
phys.atmol.lande	Lande factor
phys.atmol.level	Atomic level
phys.atmol.lifetime	Lifetime of a level
phys.atmol.lineshift	Line shifting coefficient
phys.atmol.number	Atomic number Z
phys.atmol.oscstrength	Oscillator strength
phys.atmol.parity	Parity
phys.atmol.qn	Atomic quantum number
phys.atmol.qn.i	Nuclear spin quantum number
phys.atmol.radiationtype	Type of radiation characterizing atomic lines (electric dipole/quadrupole, magnetic dipole)
phys.atmol.sweight	Statistical weight
phys.atmol.term	Atomic term
phys.atmol.transprob	Atomic transition probability, Einstein A coefficient
phys.atmol.transition	Transition between states
phys.atmol.woscstrength	Weighted oscillator strength
phys.atmol.weight	Atomic weight
phys.columndensity	Column density
phys.composition	Quantities related to composition of objects
phys.composition.masslightratio	Mass to light ratio
phys.composition.yield	Mass yield
phys.density	Density (of mass, electron, ...)
phys.dielectric	Complex dielectric function
phys.dispmeasure	Dispersion measure
phys.electfield	Electric field
phys.electron	Electron
phys.electron.degen	Electron degeneracy parameter
phys.emissmeasure	Emission measure
phys.emissivity	Emissivity
phys.energy	Energy
phys.energy.density	Energy-density
phys.eos	Equation of state
phys.excitparam	Excitation parameter U
phys.gauntfactor	Gaunt factor/correction
phys.gravity	Gravity
phys.ionizparam	Ionization parameter
phys.ionizparam.coll	Collisional ionization
phys.ionizparam.rad	Radiative ionization
phys.luminosity	Luminosity
phys.luminosity.fun	Luminosity function
phys.magabs	Absolute magnitude
phys.magabs.bol	Bolometric absolute magnitude
phys.magfield	Magnetic field
phys.mass	Mass
phys.mass.loss	Mass loss
phys.mol	Molecular data
phys.mol.dipole	Molecular dipole
phys.mol.dipole.electric	Molecular electric dipole moment
phys.mol.dipole.magnetic	Molecular magnetic dipole moment
phys.mol.dissociation	Molecular dissociation
phys.mol.formationheat	Formation heat for molecules
phys.mol.qn	Molecular quantum numbers
phys.mol.quadrupole	Molecular quadrupole
phys.mol.quadrupole.electric	Molecular electric quadrupole moment
phys.mol.rotation	Molecular rotation
phys.mol.vibration	Molecular vibration
phys.polarization	Polarization degree (or percentage)
phys.polarization.circular	Circular polarization
phys.polarization.linear	Linear polarization
phys.polarization.rotmeasure	Rotation measure polarization
phys.polarization.stokes	Stokes polarization
phys.pressure	Pressure
phys.recombination.coeff	Recombination coefficient
phys.refractindex	Refraction index
phys.size	Size (not angular)
phys.size.axisratio	Axis ratio (a/b) or (b/a)
phys.size.diameter	Diameter
phys.size.radius	Radius
phys.size.smajaxis	Linear semi major axis
phys.size.sminaxis	Linear semi minor axis
phys.temperature	Temperature
phys.temperature.effective	Effective temperature
phys.temperature.electron	Electron temperature
phys.transmission	Transmission (of filter, instrument, ...)
phys.veloc	Space velocity
phys.veloc.ang	Angular velocity
phys.veloc.dispersion	Velocity dispersion
phys.veloc.escape	Escape velocity
phys.veloc.expansion	Expansion velocity
phys.veloc.microturb	Microturbulence velocity
phys.veloc.orbital	Orbital velocity
phys.veloc.pulsat	Pulsational velocity
phys.veloc.rotat	Rotational velocity
phys.veloc.transverse	Transverse / tangential velocity
pos	Position and coordinates
pos.angdistance	Angular distance, elongation
pos.angresolution	Angular resolution
pos.az	Position in alt-azimutal frame
pos.az.alt	Alt-azimutal altitude
pos.az.azi	Alt-azimutal azimut
pos.az.zd	Alt-azimutal zenith distance
pos.barycenter	Barycenter
pos.bodyrc	Body related coordinates
pos.bodyrc.alt	Body related coordinate (altitude on the body)
pos.bodyrc.lat	Body related coordinate (latitude on the body)
pos.bodyrc.long	Body related coordinate (longitude on the body)
pos.cartesian	Cartesian (rectangular) coordinates
pos.cartesian.x	Cartesian coordinate along the x-axis
pos.cartesian.y	Cartesian coordinate along the y-axis
pos.cartesian.z	Cartesian coordinate along the z-axis
pos.cmb	Cosmic Microwave Background reference frame
pos.dircos	Direction cosine
pos.distance	Linear distance
pos.earth	Coordinates related to Earth
pos.earth.altitude	Altitude, height on Earth  above sea level
pos.earth.lat	Latitude on Earth
pos.earth.lon	Longitude on Earth
pos.ecliptic	Ecliptic coordinates
pos.ecliptic.lat	Ecliptic latitude
pos.ecliptic.lon	Ecliptic longitude
pos.eop	Earth orientation parameters
pos.eop.nutation	Earth nutation
pos.ephem	Ephemeris
pos.eq	Equatorial coordinates
pos.eq.dec	Declination in equatorial coordinates
pos.eq.ha	Hour-angle
pos.eq.ra	Right ascension in equatorial coordinates
pos.eq.spd	South polar distance in equatorial coordinates
pos.errorellipse	Positional error ellipse
pos.frame	Reference frame used for positions
pos.galactic	Galactic coordinates
pos.galactic.lat	Latitude in galactic coordinates
pos.galactic.lon	Longitude in galactic coordinates
pos.galactocentric	Galactocentric coordinate system
pos.geocentric	Geocentric coordinate system
pos.healpix	Hierarchical Equal Area IsoLatitude Pixelization
pos.heliocentric	Heliocentric position coordinate (solar system bodies)
pos.htm	Hierarchical Triangular Mesh
pos.lambert	Lambert projection
pos.lg	Local Group reference frame
pos.lsr	Local Standard of Rest reference frame
pos.lunar	Lunar coordinates
pos.lunar.occult	Occultation by lunar limb
pos.parallax	Parallax
pos.parallax.dyn	Dynamical parallax
pos.parallax.phot	Photometric parallaxes
pos.parallax.spect	Spectroscopic parallax
pos.parallax.trig	Trigonometric parallax
pos.phaseang	Phase angle, e.g. elongation of earth from sun as seen from a third cel. object
pos.pm	Proper motion
pos.posang	Position angle of a given vector
pos.precess	Precession (in equatorial coordinates)
pos.supergalactic	Supergalactic coordinates
pos.supergalactic.lat	Latitude in supergalactic coordinates
pos.supergalactic.lon	Longitude in supergalactic coordinates
pos.wcs	WCS keywords
pos.wcs.cdmatrix	WCS CDMATRIX
pos.wcs.crpix	WCS CRPIX
pos.wcs.crval	WCS CRVAL
pos.wcs.ctype	WCS CTYPE
pos.wcs.naxes	WCS NAXES
pos.wcs.naxis	WCS NAXIS
pos.wcs.scale	WCS scale or scale of an image
spect	Spectroscopy
spect.dopplerparam	Doppler parameter b
spect.dopplerveloc	Radial velocity, derived from the shift of some spectral feature
spect.dopplerveloc.opt	Radial velocity derived from a wavelength shift using the optical convention
spect.dopplerveloc.radio	Radial velocity derived from a frequency shift using the radio convention
spect.index	Spectral index
spect.line	Spectral line
spect.line.asymmetry	Line asymmetry
spect.line.broad	Spectral line broadening
spect.line.broad.stark	Stark line broadening coefficient
spect.line.broad.zeeman	Zeeman broadening
spect.line.eqwidth	Line equivalent width
spect.line.intensity	Line intensity
spect.line.profile	Line profile
spect.line.width	Spectral line fwhm
spect.resolution	Spectral (or velocity) resolution
src	Observed source viewed on the sky
src.class	Source classification (star, galaxy, cluster...)
src.class.color	Color classification
src.class.distance	Distance class e.g. Abell
src.class.luminosity	Luminosity class
src.class.richness	Richness class e.g. Abell
src.class.stargalaxy	Star/galaxy discriminator, stellarity index
src.class.struct	Structure classification e.g. Bautz-Morgan
src.density	Density of sources
src.ellipticity	Source ellipticity
src.impactparam	Impact parameter
src.morph	Morphology structure
src.morph.param	Morphological parameter
src.morph.sclength	Scale length for a galactic component (disc or bulge)
src.morph.type	Hubble morphological type (galaxies)
src.orbital	Orbital parameters
src.orbital.eccentricity	Orbit eccentricity
src.orbital.inclination	Orbit inclination
src.orbital.meananomaly	Orbit mean anomaly
src.orbital.meanmotion	Mean motion
src.orbital.node	Ascending node
src.orbital.periastron	Periastron
src.redshift	Redshift
src.redshift.phot	Photometric redshift
src.sample	Sample
src.sptype	Spectral type MK
src.var	Variability of source
src.var.amplitude	Amplitude of variation
src.var.index	Variability index
src.var.pulse	Pulse
src.veloc.hc Heliocentric radial velocity
stat	Statistical parameters
stat.fourier	Fourier coefficient
stat.fourier.amplitude	Amplitude Fourier coefficient
stat.correlation	Correlation between two parameters
stat.covariance	Covariance between two parameters
stat.error	Statistical error
stat.error.sys	Systematic error
stat.fit	Fit
stat.fit.chi2	Chi2
stat.fit.dof	Degrees of freedom
stat.fit.goodness	Goodness or significance of fit
stat.fit.omc	Observed minus computed
stat.fit.param	Parameter of fit
stat.fit.residual	Residual fit
stat.likelihood	Likelihood
stat.max	Maximum or upper limit
stat.mean	Mean, average value
stat.median	Median value
stat.min	Minimum or lowest limit
stat.param	Parameter
stat.snr	Signal to noise ratio
stat.stdev	Standard deviation
stat.value	Miscellaneous value
stat.variance	Variance
stat.weight	Statistical weight
time	Time
time.age	Age
time.crossing	Crossing time
time.epoch	Epoch, julian date
time.equinox	Equinox
time.event	Duration of an event or phenomenon
time.event.end	End time of event or phenomenon
time.event.start	Start time of event or phenomenon
time.expo	Exposure on-time, duration
time.expo.end	End time of exposure
time.expo.start	Start time of exposure
time.interval	Interval of time
time.lifetime	Lifetime
time.obs	Observation on-time, duration
time.obs.end	End time of observation
time.obs.start	Start time of observation
time.period	Period
time.phase	Phase
time.relax	Relaxation time
time.resolution	Time resolution
time.scale	Timescale


#
# The strings not very often used
#
FMSCRIPTEX	# load SuperCOSMOS H-alpha image\n$3_halpha = get SHS(H-alpha) $1 $2 5'\n# load SuperCOSMOS Short Red image\n$3_red = get SHS(Red) $1 $2 5'\n# wait for the images to be loaded\nsync\n# normalize each image\n$3_halpha_norm = norm -cut $3_halpha\nsync\n$3_red_norm = norm -cut $3_red\nsync\n# compute H-alpha minus Red\nresult_$3 = $3_halpha_norm - $3_red_norm\nsync\ncm fire\nrm $3_halpha_norm\nrm $3_red_norm\nrm $3_halpha\nrm $3_red\nsync\nzoom 2/3x
FMPARAMSEX	07 55 55.5	-33 46 00	PHR0755-3346\n08 25 46.3	-40 13 52	PHR0825-4013\n16 02 20.2	-41 27 11	PHR1602-4127\n17 18 44.9	-33 15 24	PPA1718-3315\n18 18 59.2	-15 26 21	PHR1818-1526
Northup.HELP	!North up\nApply a rotation to the image or the HiPS on its astrometrical solution to orient the North direction up.\n \nThis display mode may inhibit some pixel functions (photometry measurements...)
Northup.HELP.fr	!Nord en haut\nApplique une rotation sur la solution astromtrique de l'image ou du HiPS afin de placer le Nord du systme de coordonnes vers le haut.\n \nCe mode de visualisation inhibe ventuellement certaines fonctionnalits d'accs aux valeurs relles des pixels (photomtrie...)
Datatree.HELP	!Data discovery tree\nThis panel is dedicated to browse, to filter, and to select the data collections that you want to load, to display and to process in Aladin. These collections represents all public astronomical data available on the net: several thousands of astromical image collections, catalogs, tables, spectra provided by the Centre de Donnes astronomiques de Strasbourg and other data providers over the world compatible with the Virtual Observatory protocols and standards. For each collection, you can select various access mode depending of the nature of the data, for instance the progressive access (HiPS), or only on a specific region, etc... You can also load derived products such as coverage (MOC) or density map associated to the selected collection.\n \nThe text field and the popup menu below allow you to filter the collections that you want to display in the tree. The "+" button on the righ side of the predefined filters will allow you to create your own filters based  on key words, or any constraints spatial, temporal or numeric.\n \nThis panel can be extended or reduced by using on the right margin.
Datatree.HELP.fr	!Arbre de dcouverte\nCe bandeau permet l'affichage, la consultation, le filtrage et la slection des collections de donnes que vous souhaitez charger, afficher et manipuler dans Aladin. Il s'agit de la quasi totalit des donnes astronomiques publiques disponibles, ce qui reprsente plusieurs milliers de collections d'images astronomiques, de catalogues, de tables, de spectres issues du Centre de Donnes de Strasbourg ainsi que des autres fournisseurs de donnes mondiaux supportant les standards et protocoles de "l'Observatoire Virtuel". Pour chacune de ces collections, vous pourrez choisir parmi plusieurs moyens d'accs suivant la nature des donnes, par exemple en mode d'affichage progressif (HiPS), ou recouvrant uniquement une rgion spcifique, etc... Vous pourrez galement charger d'ventuels produits drivs tels que la couverture (MOC), ou la carte de densit associ  la collection dsigne.\n \nLe champ de saisie et les menus droulants ci-dessous vous permettront de filtrer les collections que vous souhaitez afficher. Le bouton "+"  gauche des filtres dj prdfinis vous permettra de crer vos propres filtres bass sur des mots cls, ou sur des contraintes spatiales, temporelles, ou numriques.\n \nCe panneau est extensible ou rtractable en agissant sur la marge de droite qui le spare du panneau principal.
Help.HELP	!Help on line\n*Just move the mouse on any Aladin components\n*for which you want some explanations.\n \n \n*To quit the help mode, click anywhere\n \n!Interface vocabulary\n- View window: the main window in the center of the Aladin window,\n- Plane stack: window on the right side of the Aladin window,\n- Discovery data tree: the left panel displaying available collections\n- Tool bar: the set of the logos between the View window and the Plane stack,\n-Zoom window: the square window at the right-bottom corner,\n- Measurement window: the rectangular window at the bottom of the Aladin window (retractable).
Help.HELP.fr	!Aide interactive\n*Dplacez simplement votre souris\n*sur n'importe quelle composante d'Aladin\n*afin d'obtenir de l'aide.\n \n \n*Pour quitter l'aide intractive, cliquez n'importe o\n \n!Vocabulaire\n- Fentre des vues: le panneau principal au centre de la fentre Aladin,\n- L'arbre de dcouverte: le bandeau  gauche\n- La pile des plans: le panneau  droite avec le logo en forme d'oeil,\n- la barre d'outils: les boutons entre le panneau des vues et la pile,\n- Le panneau du zoom: le carr en bas  droite,\n- Les mesures: le panneau en bas de la fentre (rtractable).
View.HELP	!View window\nDisplays the current view(s) (images + catalogs and graphical overlays) according to the status of the "Plane stacks" and the "Zoom window".\n \nThe mouse position in astronomical coordinates is given at the top of the window.  If the mouse position is on a catalog source, its name is given in the ``status window''.\n \nYou can select an individual source by clicking on it, or several sources by delimiting a rectangular area with a clik-and-drag mouse operation. All measurements and links associated to these sources will be displayed in the "Measurement window".\n \nIn the same way, you can select one or several additional graphic symbols that you can subsequently move or delete.\n \nThe "view frame" can be splitted in 2, 4, 9 or 16 panels, each one containing its own view. See the "Multiview controler" at the left-bottom side
View.HELP.fr	!Fentre de vue\nProjette la ou les vues courantes (images + catalogues + surcharges graphiques) en fonction de l'tat de la "pile des plans" et du zoom.\n \nLes coordonnes astronomiques correspondantes  la position de la souris sont indiques au-dessus de la fentre. Si la souris se trouve sur un objet issu d'un catalogue, son nom s'affiche dans le bandeau du statut.\n \nVous pouvez slectionner individuellement des objets en cliquant simplement dessus, ou en les englobant dans une slection rectangulaire. Toutes les mesures et liens associs seront alors affichs dans le "Panneau des mesures".\n \nVous pouvez galement slectionner des surcharges graphiques pour les dplacer ou les supprimer.\n \nLa "Fentre de vue" peut tre subdivise en 2, 4, 9 ou 16 panneaux, chacun contenant sa propre vue. Voir le "Controleur de multivues" en bas  gauche.
LCoord.HELP	!Localization window\nDisplays the coordinates and the pixel value corresponding to the current position of the mouse in the "View window".\nYou can choose the coordinate reference system from the menu on the left of the coordinates. Also, you can specify if Aladin will display the true pixel value or only the grey 8 bit level.\n \nYou can copy/paste the last position pointed in the view, respectively the pixel value. Click into the view, and "catch/copy" the value which has been memorized into the position window (respectively the pixel window).\n \nThe position window can be also used for executing a script command (see menu "Help -> Help on Aladin script commands"). And notably, you can write an object name or coordinates to move the reticle to the corresponding location.
LCoord.HELP.fr	!Bandeau de localisation\nAffiche les coordonnes et la valeur du pixel correspondant  la position courante de la souris dans la "Fentre de vue".\nVous pouvez modifier le systme de coordonnes au moyen du menu droulant qui se trouve sur la gauche (J2000, B1950...). De mme vous pouvez demandez l'affichage de la vraie valeur du pixel ou simplement le niveau de gris 8 bits.\n \nVous pouvez  tout moment Copier/Coller la dernire position, respectivement valeur de pixel, pointe dans la vue. Cliquez dans la vue, puis attraper/copier la valeur qui a t mmorise en vous dplacement sur le bandeau de position, puis en cliquant dessus.\n \nLe rectangle o apparat la coordonnes courantes peut servir de manire alternative  passer une commande script (voir Menu "Aide -> Aide sur les commandes en ligne"). Entre autres vous pouvez saisir directement un nom d'objet ou des coordonnes pour demander  Aladin de dplacer le rticule  la position correspondante.
MCanvas.HELP	!Measurement window\nDisplay associated data on the sources selected in the "View window".\n \nIn the "View window", you can select an individual source by clicking on it, or several sources by delimiting a rectangular area with a click-and-drag mouse operation.\n \nIn the "Measurement window" :- Move the mouse to each data component to see its label and some explanations (in the "Status window"), and to see  its corresponding source (blinking in the "View window").\n \n- Click on colored triangles at the beginning of each line to launch a Web browser and to receive explanations on the origin of the data.\n \n- Click on blue underlined components to learn more about the source.\n \nTo free this window, you have to deselect the sources by clicking in the "View window" away from all sources.\n \nTo select all the sources in a source plane, you can use the dedicated popup-menu from the "plane stack".\n \nFor your help, you can underline a measure line just by clicking on in order to easily read a long line.
MCanvas.HELP.fr	!Panneau des mesures\nAffiche les informations associes aux objets slectionns dans la "fentre de vue".\n \nDans la "fentre de vue", vous pouvez slectionner individuellement un objet en cliquant dessus, ou en slectionner plusieurs en les englobant dans une zone rectangulaire.\n \nDans le "panneau des mesures" :-Dplacez la souris sur chaque lment afin d'en connatre l'intitul et l'unit (dans le "bandeau de statut") et visualiser la source correspondante (clignote dans la "fentre de vue").\n \n- Cliquez sur le tirangles colors au dbut de chaque ligne afin d'afficher dans votre navigateur une page dtaillant l'origine des donnes.\n \n- Cliquez sur les lments en bleu souligns afin d'ouvrir votre navigateur Web avec des informations associes.\n \nPour librer la fentre vous devez simplement dselectionner les objets en cliquant sur une zone vide dans la vue.\n \nPour slectionner tous les objets dans plan catalogue, vous disposez d'un menu contextuel dans la "Pile".\n \nVous pouvez souligner une ligne de mesure en cliquant dessus afin de pouvoir aisment lire une longue ligne.
Select.HELP	!Plane stack\nControl the views of planes. A plane can be an image, a data chart, can memorize graphical overlays, iso-contour drawings, FoV or even filters. The eye of the observer is at the top of the stack and sees the projection of all active planes in the "view window" The status of a plane is specified by a little colored signal to the right of its name.\n \n- Click on a plane icon to activate it in all compatible views.\n- Click on a plane name to select it; then the tool buttons which are authorized for this kind of plane are activated. Maintain the Shift key to select several planes together\n- Click and drag the plane icons to change the order of the display in the stack. if the image is on the top, the sources are not visible but can always be selected.\n \nIn multiview mode (see "multiview controller") you can create several views of one or several planes by clicking/moving the plane icon from the "stack" into the selected view, especially a image plane.\n \nYou can organize the "stack" by using folders (popup menu available by pressing the right mouse button in the stack).\n \nYou can totally free the "Stack" by pressing the SHIFT key and simultaneously by clicking the "Del" button.
Select.HELP.fr	!La Pile\nPermet le contrle des vues de plans. Un plan peut tre une image, une carte de champs, peut contenir des lements graphiques, des iso-contours, des champs instrumentaux ou mme encore des filtres. L'oeil de l'observateur se trouve en haut de la pile et visualise la projection de tous les plans dans la "fentre de vue". Le statut de chaque plan est indiqu par une petite "balle" colore  droite du nom du plan.\n \n- Cliquez sur l'icne du plan ( gauche du nom) pour l'activer (resp. le dsactiver) dans tous les vues compatibles.\n- Cliquez sur le nom du plan pour le slectionner; les boutons des outils compatibles avec ce type de plan sont alors disponibles. Maintenez la touche MAJ pour slectionner simultanment plusieurs plans.\n- Cliquez et dplacer l'icne d'un plan pour changer son ordre dans la pile. Si l'image est au-dessus, les objets ne sont plus visibles dans la vue associe, mais toujours slectionnables.\n \nLorsque le mode multivue est actif (voir le "Controleur multivue"), vous pouvez crer plusieurs vues, d'un ou plusieurs plans, en cliquant-glissant l'icne du plan dans le panneau de la vue souhaite, typiquement une image.\n \nVous pouvez organiser la "Pile" en utilisant des rpertoires (menu contextuel accessible par le bouton droit de la souris)\n \n.Vous pouvez vider totalement la "Pile" en maintenant la touche MAJ appuye et en cliquant sur le bouton "Suppr".
Status.HELP	!Status window\nDepending on the current position of the mouse, this window displays corresponding information and/or the status, such as :\n \n- the task associated with a tool button,\n- the identifier of a source,\n- the status of a plane,\n- the size of a vector,\n- the legend associated with a measurement,\n- ...
Status.HELP.fr	!Bandeau de statut\nCe bandeau affiche de l'information en fonction de la position courante de la souris. Ainsi :\n \n- la tche associe  chaque bouton d'outil,\n- l'identificateur d'un objet,\n - le statut d'un plan,\n- la taille d'un segment de mesure,\n la lgende associe  une ligne de mesure,\n- ...
ZoomView.HELP	!Multi-functions\nThis panel is dedicated to additional information for a better analyze of the displayed data. This panel can host various graphics:\n - Zoom: visualization of the current view compared to the global image, or compared to the full spatial reference (HiSP). In this last case, a popup menu is displayed allowing to consult and reuse previous localization;\n - Histogram: distribution of the values associated to the selected catalog sources (since the mouse pointer is placed over a source measurement column);\n - SED: scatter plot in wavelength versus energy for a specific target designated by the tool "Study";\n - Pixel distribution : histogram of the pixels selected via a photometry tool ("Phot" or "Draw");\n - Cut graph: Pixel distribution along a segment (tool "dist");\n - Wen: pixel table around the current mouse position;\n - Spectra: visualization of the spectra generated from a cube (tool "spect.").\n \n This panel can be easily extended by moving the left and bottom area thanks via a clic&drag action on their border.
ZoomView.HELP.fr	!Multifonction\nCet emplacement est destin aux informations complmentaires pour comprendre et analyser les donnes en cours d'affichage. Elle peut abriter diffrents graphiques:\n - Zoom : reprage du champ courant en fonction de l'image globale, voire du rfrentiel spatial gnral (HiPS). Dans ce dernier mode, l'historique des positions dj visites est disponible sous la forme d'un menu droulant;\n - Histogramme : graphique de distribution des valeurs associes aux sources slectionnes (lorsque la souris survole te telles mesures);\n - SED : nuage de points en longueur d'ondes / nergie pour un objet astronomique repr par l'outil "Examen";\n - Distribution des pixels : histogramme de la valeur des pixels slectionns par un outil photomtrique (outil "phot" ou "dessin");\n - Graphe de coupe : Distribution des valeurs des pixels le long d'un segment (outil "dist");\n - Loupe : tableau des valeurs de pixels sous et proche de la position de la souris;\n - Spectre : affichage du spectre extrait d'un cube (outil "spect.").\n \nCette fentre peut tre aisment agrandie en dplaant (clic&drag) horizontalement et verticalement les znes sensibles des bandeaux gauche et bas.
Search.HELP	!Search/select field\nAllows the user to select the astronomical sources in the activated catalog planes for which the search string is found in their associated measurements. The two small arrows allows to highlight each sources (highlighted line + reticle position)\n \nWithout validating the search string by ENTER, you can highlight specifical sources amongst the sources previously selected.\n \nFor focusing, the string can be precedded by a column name followed by a boolean operator (=,!=,>,<,>=,<=), and possibly embedded between abs. character (|). A column name and/or a string can used "*" and "?" wildcards. The search is case insensitive.\n \nA few examples:\n \n star    : select sources containing the word "star"\n otype=uv : same but restricted to "otype" column, "ub" value\n mag*>=12 : column name starting with 'mag", value >= 12\n |pm*|<5  : column name starting with "pm", absolute value only considered\n type!=g* : "type" column for which the values do not start with "g"\n bmag!="" : none empty "bmag" column 
Search.HELP.fr !Champ de recherche/slection\nPermet  l'utilisateur de slectionner, parmi tous les plans catalogues dj chargs et activs, les sources astronomiques qui contiennent dans leurs mesures la chaine de texte indique. Les deux flches de part et d'autre du champ de saisie permettent de reprer/montrer chaque source (surbrillance+dplacement du rticule).\n \nIl est possible de saisir une chaine de recherche sans la valider (par ENTER) permettant ainsi de reprer/montrer des sources particulires parmi celles dj prsentes dans la table.\n \nPour affiner la recherche, le texte peut tre prcd d'un nom de colonne suivi d'un oprateur boolen (=,!=,>,<,>=,<=), et ventuellement encadr par des barres de valeur absolue (|). Un nom de colonne ou une chaine de recherche peut utiliser les jokers "*" et "?". Il n'y a pas de distinction majuscules/minuscules.\n \nQuelques exemples:\n \n star     : slection des sources contenant le mot "star"\n otype=uv : idem pour une colonne "otype" de valeur "uv"\n mag*>=12 : nom de colonne commenant par "mag" de valeur > 12\n |pm*]<5  : nom de colonne commenant par "pm", calcul en val.absolue\n type!=g* : la valeur de la colonne "type" ne doit pas commencer par "g"\n bmag!="" : colonne "bmag" non vide
Lock.HELP	!Lock on reticle\nClick on this icon to lock the view on the reticle.\n \nThe "lock" behavior is interesting notably in multiview mode or if the view does not show all the image (depending of the zoom factor and the image size and the Aladin frame size in the screen). In this case, a locked view will always try to display the current reticle (large magenta cross) at the center of the view by moving the field of view automatically.\n \nAssociated with the usage of the measurement search function, it provides a powerfull mechanism to quickly browse a list of targets.
Lock.HELP.fr	!Verrouillage sur le rticule\En cliquant sur cette icne, vous verrouillez la vue courante sur le rticule\n \nLa fonction "lock" est particulirement intressante en mode multivue ou dans le cas o la vue ne montre qu'une portion de l'image (fonction du facteur du zoom, de la taille de l'image et de la taille de la fentre Aladin). Une vue verrouille se centrera automatiquement sur la position courante du rticule (dans la mesure du possible).\n \nSon usage conjoint avec la fonction de recherche dans les mesures fournit un outil trs puissant pour passer en revue rapidement une liste de sources.
Grid.HELP	!Coordinate grid\nClick on this icon to activate or unactivate a grid of coordinates. The grid is drawn according to the current astronomical reference frame (Position selector just behind the Aladin menu)
Grid.HELP.fr	!Grille de coordonnes\nCliquez sur cette icne pour activer ou dsactivez l'affichage d'une grille de coordonnes. La grille est trace en fonction du systme du rfrence courant (slecteur "Position" juste en-dessous du menu Aladin).
Filter.HELP	!Filter\nActivate/unactivate the filtering on the data discovery tree. This function switch on/off both the quick filter based on basic key words and the advanced filters.
Filter.HELP.fr	!Filtre\nActive/dsactive le filtrage de l'arbre des collections de donnes. Ceci concerne le filtrage rapide par simple mots cls, ainsi que les filtres avancs.
Hdr.HELP	!High Dynamic Range\nSwitch between the "preview" display mode nd the "full dynamic" mode. This last mode allows you to manipulate the true pixel values (see "phot" tool), and to adjust the display contrast as you whish (see "Pixel" tool). Note that this full contraste adjustement is automatically done by default based on the center area of the current view.
Hdr.HELP.fr	!High Dynamic Range\nCliquez sur cette icne pour alterner la visualisation "previsualisation" <-> "dynamique complte" des pixels.  Le mode "dynamique complte" permet d'accder aux valeurs des pixels (cf. outil phot), et d'ajuster selon vos besoins la dynamique d'affichage (cf. outil Pixel). Cette dynamique est par dfaut automatiquement recalcule en fonction de la zone centrale de la vue.
Scan.HELP	!Scan\nDetermine if the selected collections in the data tree have or not data in the current view.\n \nThis function is only dedicated to the collections which do not provide their spatial coverage (MOC)\n \nNote that a scan is a long process, and the results only concern the current view. You will have to redo it for another field.
Scan.HELP.fr	!Scan\nDtermine les collections qui ont ou non des donnes dans le champ de vue courant.\n \nCette fonction n'a d'intrt que pour les collections qui ne fournissent pas la description de leur couverture spatiale (MOC)\n \nCette opration est longue et ne fournit qu'une rponse sur le champ courant. Vous devrez refaire l'opration pour un nouveau champ.
Collapse.HELP	!Expand/Collapse\nExpand (respectively collapse) the selected tree branches.
Collapse.HELP.fr	!Dploie/Referme\nOuvre (respectivement ferme) la ou les branches de l'arbre slectionns.
Sort.HELP	!Sort\nModify the order in the selected tree branch.
Sort.HELP.fr	!Tri\nModifie la rgle d'ordonnancement de la branche de l'arbre slectionne
Inside.HELP	!In view only\nSince this function is activated, all collections which do not have data in the current field (those normally written in orange color) are no longer displayed in the data discovery tree.
Inside.HELP.fr	!Dans la vue\nLorsque cette fonction est active, les collections qui ne disposent d'aucune donne dans le champ courant (celles normalement prsentes en couleur orange) n'apparaissent plus dans l'arbre des donnes.
ViewControl.HELP	!Multiview controller\nAllows you to slip the "View Window" in 2, 4, 9 or 16 sub-panels.\n \nEach subpanel can display a specifical views (images and/or catalogs..) with its own zoom factor. \n - To put an image into a view, just clic and drag the logo from the Aladin stack (at the right of the Aladin window) into the panel\n - You select a view just by clicking into its panel (SHIFT clic to select several views). A blue border shows the current view(s).\n - If you move the mouse on the stack or on the panel views, a green border around the panels and a small green triangle in the stack shows the associations.
ViewControl.HELP.fr	!Controleur du multivue\nVous permet de diviser la "Fentre de vue" en 2, 4, 9 ou 16 panneaux.\n \nChaque panneau peut afficher une vue spcifique (images et/ou catalogues...) avec sont propre facteur de zoom.\n - Pour mettre une image dans une vue, cliquez simplement dans le logo du plan dans la pile ( droite) puis dplacez-le dans le panneau.\n - La slection d'un vue se fait simplement en cliquant dans son panneau (maintenez la touche MAJ pour slectionner simultanment plusieurs vues). Un bord bleu visualise la (ou les) vue courante.\n - Lorsque vous dplacez la souris sur la pile ou sur les panneaux des vues, un bord vert autour des panneaux et un petit triangle vert dans la pile montre les associations.
Sync.HELP	!View synchronisation\nThis tool can be only used in multiview mode.\n \nThe icon drawn with a green background specifies that at least two views have a common sky area. By clicking on the icon, all compatible views will be automatically adjusted for displaying the field of the current view (same center and zoom factor adjusted for displaying the same sky area).\n \nThe icon will be drawn with a red background specifying that all compatible views are currently selected and can be manipulated together for zooming, panning.... Click again the icon for deselecting the other views.
Sync.HELP.fr	!Synchronisation des vues\nCet outil ne peut tre utilis qu'en mode multivue.\n \nL'icne verte indique qu'au moins deux vues ont une portion du ciel en commun. En cliquant sur l'icne, toutes les vues compatibles vont s'ajuster pour montrer le mme champ de vue que celui de la vue courante (mme centre et facteur de zoom ajust pour afficher la mme portion du ciel).\n \nL'icne passe en rouge pour indiquer que toutes les vues compatibles sont actuellement slectionnes et peuvent tre manipules en groupe (zoom, pan...). Cliquez  nouveau sur l'icne pour deslectionner les vues additionnelles.
Look.HELP !Study\nLook for details on the object under the mouse\nThis tool allows to query the astronomical Simbad data base to get the identifier and the basis measurements of the object the most studied under the mouse position (orange mode icon).\n  \nThis tool can be coupled with the VizieR catalog service to generate an histogram of the photometric measurements found in the catalogs containing information on this position (green mode icon).
Look.HELP.fr  !Examen\nExamen de l'objet sous la souris\nL'activation de cet outil permet d'interroger la base de donnes astronomique Simbad afin de rcuprer l'identificateur et les paramtres fondamentaux de l'objet astronomique le plus tudi qui se trouve sous la souris (mode icne orange).\n \nCet outil peut galement tre coupl au service des catalogues VizieR afin de gnrer un graphe des mesures photomtriques rpertories dans l'ensemble des catalogues qui contiennent un objet autour de cette position (mode icne verte).
ToolBox.HELP1	!Tool bar\nDisplay all of Aladin tools. Depending on the selected plane in the "plane stack", only the tools adaptated to this plane type will be activated. If there are several "selected planes", only tools adaptated to all of them will be activated. The "Select" tool is activated by default.
ToolBox.HELP1.fr	!Barre d'outils\nAffiche tous les outils Aladin. En fonction du plan slectionn dans la "pile", seuls les outils adapts  ce type de plan seront activs. S'il y a plusieurs plans slectionns, seuls les outils adapts  tous ces plans seront activs.  Le bouton "Select" s'active par dfaut.
ToolBox.HELP2	!Proportion modifier\nBy dragging this logo, you can alter the relative proportions of Aladin components. You can also use the "Split" button to detach totally the "measurement frame".
ToolBox.HELP2.fr	!Modificateur de proportion\nEn dplaant ce logo, vous pouvez modifiez les proportions relatives des diffrents composantes d'Aladin. Vous pouvez galement utiliser le bouton "Split" pour dtacher totalement le "panneau des mesures".
Tool.select	The "selector" is the default tool. It's goal is to allow you to select one or several objects in a "view". To do so, just click on an object (catalog source or graphic symbol) or enclose them with a rectangle. For all selected sources, the associated measurements are displayed in the "Measurement window".\nYou can modify the current selection by holding down the SHIFT key during a new selection.\nTo unselect all current objects, just click on a blank area.\n \nSelected graphic symbols can be moved by clicking again and dragging the mouse. Also, some FoV can rotate. For that, move the mouse on one angle of the FoV, thus, clic&drag.\n \nBy pressing the Alt key, you will temporarely switch into the Pan mode allowing you to move the visible area by clicking and dragging.
Tool.select.fr	Le "slecteur" est l'outil actif par dfaut. Il vous permet de slectionner un ou plusieurs objets dans une "vue". Cliquez sur un objet (provenant d'un catalogue ou d'une surcharge graphique) ou englobez-le dans un rectangle. Pour chaque objet slectionn, les mesures associes sont affiches dans le "panneau des mesures".\nVous pouvez modifier la slection courante en maintenant appuy la touche MAJ durant la nouvelle slection.\nPour dselectionner les objets en cours de slection, cliquez simplement sur une zone vide.\n \nLes surcharges graphiques peuvent tre dplaces par glisser/dposer. De mme certains champs instrumentaux (FoV) peuvent tre pivots. Pour cela, placez la souris sur un angle du champ instrumental, puis cliquez/glissez.\n \nSi En appuyant sur la touche Alt, vous activez temporairement le mode Dpl. (Pan) afin de vous permettre de dplacer le champ de vue par un cliquer-dplacer.
Tool.draw	The "drawing" tool allows you to draw lines or curves on the "views". By holding down the mouse button while drawing, you will draw a curve; by simply clicking one line at a time, you will draw a poly-line until the mouse leaves the "views" window. To create a polygon, complete your plot by clicking one last time on the first vertex of your plot.In this case and if the image allows it, Aladdin will display the statistics of the enclosed pixels.
Tool.dessin.fr	L'outil "dessin" vous permet de tracer des lignes ou des courbes sur les "vues".\n \nEn gardant appuy le bouton de la souris durant le trac, vous dessinerez une courbe; en cliquant simplement de proche en proche, une poly-ligne jusqu' ce que la souris sorte de la fentre des "vues". Pour crer un polygone, terminez votre trac en cliquant une dernire fois sur le premier sommet de votre trac. Dans ce cas et si l'image le permet, Aladin affichera les statistiques des pixels englobs.
#Tool.text	The "Overplot text editor" allows you to add text in a view.\n \nClick on the desired position in the "View window" and type the text.
#Tool.texte.fr	L'outil de texte vous permet de placer du texte dans une vue.\n \nCliquez  l'emplacement dsir dans la vue puis saississez le texte.
Tool.phot	The "photometry marker" allows you to compute photometric estimations. A simple mouse clic draws an ellipse centered on the closest sources. Simultaneously, the extraction parameters are displayed in the measurement frame. A clic-and-drag during the marker creation will provide some statistics concerning the pixels embedded in the generated circle.
Tool.phot.fr	L'outil de "Photomtrie" vous permet de faire des mesures photomtriques localises. Un simple clic cre une ellipse centre sur la source la plus proche et fait apparatre dans la fentre des mesures les paramtres de l'extraction correspondante. Au contriaire, un cliquer-dplacer lors de la cration de la mesure fournira des valeurs statistiques sur les pixels englobs par le cercle gnr.
Tool.tag	The "Overplot marker" allows you to annotate your "View window". A simple mouse clic creates a simple tag. A clic-and-drag during the creation will allow you to insert a label. These tags can be selected and moved. Background, border, font size, and reticle type can be modified via the mouse wheel or via the small control handles.
Tool.marq.fr	L'outil de "Marquage" vous permet d'annoter vos vues. Le placement d'une marque simple s'effectue par un clic souris. Un cliquer-dplacer lors de la cration permet d'insrer un label associ  la marque. Ces marques peuvent tre slectionnes et dplaces. Le fond, le bord, la taille et le type de rticule sont modifiable soit par la molette de la souris soit par les poignes de contrle.
Tool.dist	The "Overplot measurer and Cut graph" allows you to draw vectors in the "View window".\n \nThe length of the vector is given in the "Status window" (delta RA, delta DE, size in arcmin, Angle from the North). \n \nIn parallel, a cut graph is drawn in the "zoom window" (right bottom panel) showning the pixel distribution on the vector.
Tool.spect	The "spectrum extractor" tool is dedicated to data cubes. It allows you to display the spectre along of the longitudinal cut corresponding to the selected pixel.\n \nThe extracted spectrum is displayed is the bottom right panel since you have selected the cross tag in the main view.\nThe current cube plane is represented by the vertical red bar that you can move via the mouse (clic&drag). You can also modified the position of the pixel by moving the associated cross tag (clic&drag).\n \nThe spectrum uses the visualisation pixel range of the cube. Adjust this range (pixel tool) if necessary for modifying the min and max values.
Tool.spect.fr	L'outil d'extraction de spectres est ddi aux cubes de donnes. Il vous permet de visualiser la coupe transversale  la position du pixel que vous avez slectionn.\n \nLe spectre extrait est visualis dans la fentre en bas  droite  la condition que le marqueur du pixel d'extraction soit slectionn. Le plan courant est repr par un barre verticale rouge. Celle-ci peut tre dplacer  la souris (cliquez+dplacez). Vous pouvez galement modifier la position d'extraction du spectre en dplaant le repre dans la vue (cliquez+dplacez).\n \nLe spectre reprsent utilise la dynamique de visualisation du cube. N'hsitez pas  ajuster la dynamique des pixels pour ajuster les valeurs min et max.
Tool.x-y.fr	the "scatter/time plot" tool allows you to compare two phyical metrics associated to catalog plane sources (especially the time).\n \nSince you activate this tool, a new view is created in the main panel for the graph, and you have to specify via the properties window associated to the plane which values you want to compare.\n \nNotice that you can select some points of the scatter plot for seeing where the corresponding sources are localized in the other views.
Tool.x-y.fr	L'outil "nuage de points/srie temporelle" permet de comparer deux grandeurs physiques associes aux sources d'un plan catalogue (dont le temps).\n \nL'activation de cet outil gnre une nouvelle vue pour accueillir le graphique et vous demande de slectionner les deux valeurs  tracer (via la fentre des proprits du plan).\n \nLa slection de points dans le graphe sera automatiquement reporte dans les autres vues vous permettant de reprer leurs positions spatiales.
Tool.dist.fr	L'outil de mesure vous permet de dessiner des segments dans les vues.\n \nLa taille du segment s'affiche dans le "bandeau de statut" (delta RA, delta DE, taille en minutes d'arcs et angles depuis le Nord).\n \nEn parallle, une "coupe de pixels" s'affiche dans le panneau du zoom (en bas  droite) dessinant le graphe de rpartition des pixels le long du segment.
Tool.crop	The "crop" tool allows you to extract a sub-image from the current image.\n \nSpecify the area by a clic&drag, and adjust the rectangle via the mouse or directly by clicking on the width or height fields to edit values by the keyboard.\n \nIn case of HiPS displayed in "full dynamic" mode, you can also specify the resolution either by editing the mult.factor or by selected the check box "full resolution".Take care of the final image size before launching the extraction.
Tool.coupe.fr	L'outil de "coupe" vous permet d'extraire une sous-image de l'image courante.\n \nDterminez la zone concerne par un cliqu/tendre  la souris. Vous pouvez ajuster le rectangle via la souris ou en cliquant dans les cartouches indiquant la largeur et la hauteur et saisir directement une valeur au clavier.\n \nDans le cas d'un HiPS en mode "dynamique complte", vous pouvez galement indiquer la rsolution finale souhaite, soit en cliquant dans le cartouche du facteur multiplicatif, soit sur la coche "full resolution". Vrifiez la taille de l'image gnre avant de lancer l'extraction.
Tool.del	This tool allows you to delete selected objects (see SELECT button). Only graphic symbols can be deleted ; the sources can't be cleared individually. If there are no selected objects, the current view is deleted. And if the current view is already empty or if you clicked directly on the name plane in the stack, the selected plane(s) is deleted (see the "plane stack").\n \nWith the SHIFT key pressed, all the views (respectively all the planes) are deleted\n \nWarning: there is no "undo" function.
Tool.suppr.fr	Cet outil vous permet de supprimer les objets slectionns (voir le bouton SELECT). Seules les surcharges graphiques peuvent tre supprims; les objets de catalogues ne peuvent tre effacs individuellement. S'il n'y a pas d'objet slectionn c'est la (ou les) vue slectionn qui sera efface. De mme si la vue courante est vide ou que vous avez directement cliqu sur le nom d'un plan dans la pile, c'est le (ou les) plans slectionns qui sera supprim (voir la "pile").\n \nEn appuyant simultanment la touche MAJ et le bouton SUPPR, toutes les vues (respectivement tous les plans seront effacs\n \nAvertissement : Il n'y a pas de fonction "Dfaire/Undo".
Tool.mglss	This tool actives the magnifying glass around the mouse. The "Zoom window" window shows the region in the vicinity of the mouse when it is in the "View window".\nYou can use the arrow keys to focus the pointer and the RETURN key to validate the new position (reticle)
Tool.loupe.fr	Cet outil active la loupe  l'emplacement de la souris. Le "panneau de zoom" sera utilis pour montrer la portion zoome lorsque la souris est dans la "fentre de vue".\nVous pouvez utiliser les touches de flches pour pointer prcisment une position et appuyer ENTER pour valider la nouveau position (dplacement du rticule)
Tool.prop	Opens windows with the properties of the selected planes.\nThe property window allow you to modify the plane label, the color and the shape for the sources and all other parameters associated to the plane.
Tool.prop.fr	Ouvre les fentres des proprits des plans slectionns.\nLa fentre des proprit vous permet de modifier le nom du plan, la couleur et la forme des objets et tout autre paramtre associ au plan.
Tool.moc	Opens windows for manipulating MOCs.\nThis form allows you to combine area stored as "Multi Order Coverage maps": union, intersection, addition, subtraction...
Tool.moc.fr	Ouvre la fentre de manipulation des MOC.\nCe formulaire vous permet de combiner des rgions mmorises sous la forme de "Multi Order Coverage maps": union, intersection, addition, soustraction...
Tool.xmatch	Opens X-match windows.\nThis form allows you to combine two catalog planes by correlating their sources. This X-mach can be operated based on a common field or by spatial distance, with or without error ellipse.
Tool.corr..fr	Ouvre la fentre du X-match.\nCe formulaire vous permet de combiner deux plans catalogues par corrlation de leurs sources. Cette corrlation peut tre oprer par un champ commun ou par distance spatiale, avec ou sans ellipse d'incertitude.
Tool.pan	This tool allows you to move the visible area of the image by a simple click-and-drag. A click-and-drag-and-throw (a la google earth) initiate an automatical scrolling.\n \nPressing the SHIFT key will synchronize all views by adjusting their zoom factor and position in order to display the same sky area.\n \nAs the "select" tool, the mouse wheel allows you to change the current zoom factor.
Tool.dpl..fr	Cet outil permet de dplacer la partie visible de l'image dans la vue par un simple cliquer-dplacer. Il est galement possible d'initier un dplacement automatique par un cliquer-dplacer-jeter ( la google earth).\n \nL'usage de la touche MAJ entranera la synchronisation des vues qui ajusteront leur facteur de zoom et leur position pour afficher la mme zone du ciel.\n \nComme pour l'outil "Select", la molette de la souris permet de modifier le facteur de zoom. 
Tool.zoom	This tool allows you to zoom in the view. By using the left button, you will zoom forward on the mouse position, by clicking the right button, you will zoom backward
Tool.zoom.fr	Cet outil vous permet de zoomer dans la vue. Le cliquet de gauche augmente le facteur de zoom et centre la rgion sur la position de la souris. Le cliquet de droit diminue le facteur de zoom.
Tool.pixel	This tool allows you to enhance the current image by modifying the dynamic of the color map :\n.Use the transfer functions (log, sqrt, linear, sqr) for modifying globally the contrast.\n.Move the left triangle towards the right to suppress the background noise\n.Move the right triangle towards the left to enhance the objects\n.Adjust the last triangle according to the gray histogram to enhance the intermediate gray levels\n.Reverse the gray levels by pressing the REVERSE button or choose another color map.\n \nYou can also modify the min and max pixel range.
Tool.pixel.fr	Cet outil vous permet d'amliorer l'image courante en modifiant la dynamique de sa table des couleur:\n.Utilisez les fonctions de transfert (log, sqrt, linear, sqr) pour modifier globalement le contraste.\n.Dplacez le petit triangle de contrle de gauche pour supprimer le bruit de fond.\n.Dplacez le petit triangle de contrle de droite pour amliorer le rendu des objets\n.Ajuster le triangle du milieu pour amliorer les niveaux de gris intermdiaires.\n.Inversez les pixels en activant le bouton "Inverse" ou appliquez une autre table des couleurs.\n \nVous pouvez galement modifier la limite minimale et maximale des pixels pris en compte.
Tool.cross	This tool allows you to cross-match sources of two catalogues loaded in the Aladin stack. The cross-match can be done either by distance or by cross-ID or by positional ellipses. This operation will generate a new catalogue plane containing the cross-matched sources associated with the original catalog selected fields. One million source cross-match is not a problem and will take one or two minutes.
Tool.corr.fr	Cet outil vous permet de corrler les sources de deux catalogues pralablement chargs dans la pile Aladin. La corrlation peut tre base soit sur la distance entre les sources, soit par recouvrement des ellipses positionnels, ou encore par valeur d'une champ particulier. A l'issu de cette opration, un plan catalogue rsultat est gnr contenant les sources corrles associes aux champs des deux tables d'origines qui auront t retenus. La corrlation d'un million de sources ne pose pas de problme particulier et est effectue en quelques dizaines de secondes.
#Tool.rsamp	This tool allows you to resample all selected images according to an unique astrometrical solution. For each resampled image, a new plane is automatically created and the original one can be kept.
#Tool.rsamp.fr	Cet outil vous permet de rchantillonner toutes les images slectionnes en fonction d'une mme solution astromtrique. Pour chaque image cre, un nouveau plan est automatiquement insr dans la pile. Le plan de l'image originale peut tre conserv.
Tool.rgb	This tool allows you to create a colored RGB image. An RGB image is a composed image built with three other images already loaded in the plane stack.\nThe resampling used to do that is based on the nearest pixel position.
Tool.rvb.fr	Cet outil vous permet de crer une image couleur RVB. Une image RVB est une image composite construite  partir de trois autres images dj charges dans la pile.\nLe rchantillonnage utilis pour effectuer cette composition est bas sur l'algorithme du plus proche pixel.
Tool.cont	This tool allows you to plot contours in the image according to the grey levels you choose.
Tool.cont.fr	Cet outil vous permet de calculer et tracer les iso-contours de l'image courante en fonction des niveaux de gris que vous aurez choisis.
Tool.filter	This tool allows you to constraints the overlayed object characteristics (shape, color, hidden/shown,...) by defining a "filter" plane.
Tool.filtre.fr	Cet outil vous permet de contraindre la manire dont les objets issus de catalogues vont tre affichs (forme, couleur, cach/montr) en dfinissant un plan "filter"
Tool.assoc	This tools allows you to create an image association: either a blinking sequence or a mosaic of images. This association is composed of several images built with 2 or more images already loaded in the stack.\n \nAll images will be resampled on a same astrometrical solution.
Tool.assoc.fr	Cet outil vous permet de crer une assocation d'images : soit une squence anime, soit une mosaique. Il s'agit d'afficher 2 ou plusieurs images dans une mme vue. Ces images doivent avoir t au pralable charges dans la pile.\n \nToutes les images de l'association vont tre rchantillonnes en fonction d'une unique solution astromtrique.
Tutorial.Show-me-how-to-load-an-image	demo on \n info First of all press the "Open" button in the menu bar, and after that fill in the image server form displayed when you click on an image server button (left side), for example "Aladin" \n get Aladin(SERC/S/MAMA) M16 \n demo end\n
Tutorial.Show-me-how-to-display-catalogs-on-an-image	demo on \n info We will work on a DSS image of M101 coming from SkyView image server \n get SkyView(DSS2,600) M101; sync ; zoom 2x \n info And now we will query Simbad for this field \n get Simbad M101; sync \n info Perhaps there are also NED data ? \n get Ned M101 \n info And for the end, let's load the GSC1.2 catalog and the HST log from VizieR server \n get Vizier(GSC1.2) M101 \n get VizieR(HST) M101; sync \n now you can select any object just by clicking on it. You will see the corresponding measurements for each of them. \n info If you click on the blue underlined words in the measurements, Aladin will open your favorite navigator to show you additionnal information (full record, related bibliography,...) \n info In case of a log mission such as HST, you will be able to load directly image previews via a button directly inserted in the measurement \n demo end\n
Tutorial.Show-me-how-to-play-with-the-Aladin-stack	demo on \n info Let's work on M104 object... \n demo off \n get aladin(low) M104; get aladin M104; get Simbad M104; get NED M104; get Vizier(2MASS) M104; get VizieR(USNO2) M104; sync \n demo on \n info Each result arrives in an indidual "plane". You will see the full result as a "stack" of slides \n info You can switch off/on each of them just by clicking on the logo in front of the plane label \n hide Simbad \n hide NED \n hide Lw-* \n hide USNO2 \n show USNO2 \n info you can change the background image also by clicking on its plane logo\n show Lw-* \n pause 1 \n show DSS* \n pause 1 \n show Lw-* \n pause 1 \n show DSS* \n info You can set together some planes in a folder via the stack popup menu \n md MyFolder  \n mv DSS* MyFolder \n mv Simbad MyFolder \n mv NED MyFolder \n info Have a look in this stack popup menu by right clicking anywhere in the stack panel. \n demo end\n
Tutorial.Show-me-how-to-use-the-multiview-mode	demo on \n info Aladin can visualize several views in parallel. For example, we will load a DSS image of M101... \n demo off \n get aladin M101; sync \n demo on \n info Now we will split the view frame in several panels just by clicking on the corresponding multiview controller logo (bottom left)... \n modeview 4 \n info You can create a new view of the same image... Just click and drag the plane logo of the image in the aladin stack to a free view panel \ncreateview 1 A2\n14:03:45.94 +54:21:51.6\nzoom 2x\n info By default, each new image loaded in Aladin will be displayed in a new view panel \n demo off \n get NVSS ; sync \n demo on \n info If you select simultaneously several panels by shift-clicking them, a zoom modification (position or factor) will be applied simultaneously on each view \n select A2 B1\n zoom 4x\n pause 2\n zoom 2x\n info Notice that you can use more than the visible panels. Use the left scrolling bar to access additional panels...\n info All graphical overlays will be simultaneously drawn on each view. Suppose that we extract a contour on the first image... \n demo off \n select 1; contour \n demo on \n Have a look on the Aladin manual for other multiview facilities \n demo end\n
Tutorial.Show-me-how-to-do-a-contour	demo on \n info How to do a contour ? \n info First of all, load an image.. \n get aladin m101 \n sync \n info and press the "Cont" button in the tool bar... \n contour \n demo end\n
Tutorial.Show-me-how-to-create-a-colored-image	demo on \n info How to create a colored image ? \n info You need at least 2 images \n get aladin(POSSI/E/DSS1) M101 \n get aladin(POSSII/J/DSS2) M101 \n get aladin(POSSII/N/DSS2) M101 \n sync \n info Now press the RGB button in the Aladin toolbar... \n rgb 1 2 3 \n sync \n info You can eventually adjust the constrast of each color component by the "Hist" button. \n demo end\n
Tutorial.Show-me-how-to-control-the-image-contrast	demo on \n info We are going to load an image \n get aladin M88 \n info You have to press the "Hist" button in the Aladin toolbar \n info and adjust the constrast by the transfer functions (log, linear...) or other available possibilities \n info For example, we can change the color map and reverse the video \n cm BB \n reverse off \n demo end\n
Tutorial.What-is-a-filter	demo on \n info A filter in Aladin allows you to constraint the object overlay display \n info First of all, we are going to load USNO objects on NGC6946 field \n demo off \n get Aladin NGC6946 \n get VizieR(USNO-B1) NGC6946 ; sync \n demo on \n info Now we are going to keep only the objects for which the magnitude are less than 16 \n info To do that, we will create this filter \n filter MyFirstFilter { ${B1mag}<16 { draw } } \n demo off \n hide 1 \n pause 1 \n show 1 \n pause 1 \n hide 1 \n pause 1 \n show 1 \n demo on\n info A filter is based on this syntax: "condition { action }" \n info You can prefer to use UCD column designations instead of the column names in order to use this filter with several heterogeneous catalogs \n info For example, if we load GSC2.2 catalog... \n get Vizier(GSC2.2) NGC6946 \n demo off \n mv GSC2.2 MyFirstFilter \n demo on \n info As you can see, this filter can not match the GSC catalog as the magnitude column has not the same name \n demo off \n hide MyFirstFilter \n pause 1 \n show MyFirstFilter \n pause 1 \n hide MyFirstFilter \n pause 1 \n show MyFirstFilter \n demo on \n info Now, rewrite this filter with the UCD associated to the magnitude $[PHOT*] \n demo off \n rm MyFirstFilter \n demo on \n filter MyUCDFilter { $[PHOT*]<16 { draw } } \n info As you can see, this filter matches both GSC and USNO catalog \n hide 1 \n pause 1 \n show 1 \n pause 1 \n show 1 \n You can know all column names and all available UCDs via a popup menu in the filter text field (right click) \n info The filter actions can be more complex than a simple "draw". Try a circle \n demo off \n rm MyUCDFilter \n demo on \n filter MyCircleFilter { $[PHOT*]<16 { draw circle(10) } } \n info The action can have variable parameters, for example, a circle proportional to the magnitude \n demo off \n rm MyCircleFilter \n demo on \n filter MyPropCircleFilter { $[PHOT*]<16 { draw circle(-$[PHOT*]) } } \n info You can see the available actions in the filter popup menu.\n info You can also choose one of the predefined filters for drawing ellipses, proper motion arrows... \n demo off \n get simbad NGC6946 \n MyPropCircleFilter \n filter Prop.Motions { $[PHOT*]<18 { draw pm(0.2*$[pos.pm;pos.eq.ra], 0.2*$[pos.pm;pos.eq.dec]) } } \n filter Ellipses { { draw ellipse(0.5*$[phys.angSize.smajAxis],0.5*$[phys.angSize.smajAxis],$[pos.posAng]) } } \n filter on \n demo on \n info A not so trivial syntax but for a powerful tool, isn't it ? \n demo end\n
Tutorial.Show-me-how-to-play-with-the-metadata-lists-and-trees	demo on \n info Some image servers can provide lists of available images for a given field (called "meta data" information) \n info Let's work on Trifid region \n demo off \n get aladin(MAMA,S,PLATE) Trifid \n zoom 1/2x \n demo on \n info You can ask the Aladin server to provide all available images around a position as a list or a tree\n get aladin(2MASS/J) 18 02 19.5 -22 51 06.8 \n info When you move your mouse through this list, you see on the current view the field covered by the other images \n info Aladin can also dynamically scan a directory of your disk to build a list or tree of your own available images and catalogs \n info Let's see your current directory \n get Local(.) \n info Aladin can also display as a tree (or list) the history of your queries \n info Click on the "History" item in the File menu... \n demo end\n
Help.[name=]	#n:Plane name advanced usage#s:planeName = command...#d:Some Aladin script commands can be preceded by a plane name. In this condition the result of a such command will be stored in a new plane called by the specified "name". If this plane is already existing, the result will overwrite the previous plane contain.\n \nUsing these plane mechanism, you are able to use Aladin as a "processor" for which the "variables" are the planes.#e:A = @get ESO(dss1) m1\nB = @conv A edge\nC = B @- A\nC = @flipflop C
Help.get	#n:_get_ - call a remote image or tabular data server#s:@[name=] get Server([paramname=]keyword,...) [Target] [RadiusUnit]#d:Allows one to query remote data providers. The result (images or tabular data) will be memorized in an Aladin stack plane and a view of this plane is automatically created. The get syntax is flexible in order to cover all kinds of servers.\n   - Server:  Aladin, Simbad, VizieR, NED, SkyView, DSS.ESO, DSS.STScI, ..., or even Fov or File (or any other server names displayed in the server frame). Each server name can be followed by a comma separated keyword list in parentheses (optionally precedeed by "paramName="). The number and order of the keywords does not matter. Aladin tries to automatically associate the keywords with the server query vocabulary. \n   -Target: astronomical object identifier or J2000 coordinates in sexagesimal syntax (with blank separator). By default, Aladin takes into account the last specified target.\n   -Radius: must be specified with units (deg,arcmin,arcsec or  ' ") with no blanks between the figures or the units. By default, Aladin takes the most appropriate radius according to the current view.#e:get Aladin M99#e:get ESO(DSS2,FITS) M1 10'#e:get SkyView(pixels=800,Survey=2MASS) M1#e:foo=get File(http://myserver/myfile)#g:@load, @show, @cview, @setconf timeout=...
Help.load	#n:_load_ - load a file#s:@[name=] load filename#s:@[name=] load url#d:Allows loading of a local or remote file containing either an image, a catalog or any other data type used by Aladin.\n \nThe contents of the file is automatically detected by Aladin. The file may be gzipped.\n \nIf the filename specifies a directory, Aladin automatically creates a MetaData Tree describing all the data in the directory and its sub-directories.\nA "metadata file" describes a set of data\n \nThe supported formats are:\n   -Images: FITS, Jpeg, PNG, MEF, Healpix maps\n   -Tabular data: TSV, CSV,  VOTable, FITS, S-extractor, CSV-Excel, ASCII\n   -MetaData tree: SIA, IDHA\n   -Script: Aladin script (.ajs), DS9 regions (.reg)\n   -Backup: Aladin stack backup (AJ extension)\n   -Healpix dir: directory containing Aladin Healpix tree\n   -Glu dic: GLU server form description#e:load DSS1-M1.fits.gz#g:@get, @export, @save, @backup
Help.save	#n:_save_ - save the current view#s:save [-eps|-jpg[NN]|-png] [-lk] [WxH] [filename]#d:Save the current view (image+overlays) in a file (BMP format by default or EPS, JPEG or PNG). The parameter -eps (resp. -jpg or -png) is optional if the proper filename extension is used (.eps, .jpg or .png). The jpg parameter can be followed by a quality indicator [0..100]. The astrometrical calibration is conserved for FITS, JPEG and PNG. In multiview mode, only the selected view will be saved.\nThe -lk parameter generates an associated Tab-Separated-Value file (extension ".lk") containing the XY image coordinates, identifier and HTTP url for each overlaying astronomical source. This feature is dedicated for creating a clickable web map" page (see FAQ)\n \nThe dimension of the output image can be specified (in pixels) only in "nogui" mode (Aladin session with no graphical interface (-nogui command line parameter). Use -1x-1 for avoiding any resizing. Also in nogui mode, if there is no filename, the result is written on the standard output.\n#t:BMP is a simple bitmap format, JPEG is a lossy compressed format, PNG is a lossless compressed format, EPS (Encapsulated Postscript) is dedicated for publications (notably in latex documents).#e:save m1.eps#e:save -lk \home\img.png#e:save -jpg97 300x300#g:@load, @export, @backup
Help.export	#n:_export_ - save images or tabular data#s:export [-fmt] x filename#s:export -ROI filename#d:Export the plane "x" in the specify filename.\n \nThe optional "-fmt" parameter modifies the default format\n -Tables: default TSV, can be replaced by VOTable (-votable or ".xml" extension) \n -images: default FITS, can be replaced by JPEG (-jpg or ".jpg" extension)\nThe "-ROI" parameter allows you to save in several FITS files (prefixed by "filename") the ROI views.\n \nNotice : The image pixels will be truncated to 8 bits if the original pixels are not available. Also, the recorded WCS calibration will be the last one used for this image.\nThe Blink plane cannot be exported.#e:export DSS1.V.SERC C:\DSS2image.fits#e:export -votable GSC1.2 /home/gsc1.2.dat#e:export RGBimg m1RGB.fits#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#g:@load, @save, @backup, @thumbnail, @rm -ROI
Help.backup	#n:_backup_ - backup the Aladin stack#s:backup filename#d:Generate a backup of the Aladin plane stack in the specified file. The usual extension for this kind of file is ".AJ". The internal format is Aladin proprietary (XML syntax). Only image, tabular data and graphical overlays will be taken into account. The original pixels are lost: only the 8bit pixel values will be kept.#e:backup /home/M1.aj#g:@load, @export, @save
Help.zoom	#n:_zoom_ - change the zoom factor#s:zoom 1/64x|...|64x#s:zoom -|+#s:zoom radius#d:Change the zoom factor on the current view\nThe available factors are the powers of two (1/64x ... 64x) plus the 2/3 factor\n \nThe parameter + (resp. -) selects the next (resp. previous) zoom factor.\n \nIt is also possible to specify a radius with a unit (deg,arcmin,arcsec - by default in arcmin). In this case, the resulting zoom factor will be the closest available zoom factor covering this celestian area#t:The zoom command can only be applied on the current view(s)#e:zoom 2x#e:zoom 1/4x#e:zoom +#e:zoom 2 arcmin#g:select
#Help.reverse	#n:_reverse_ (un)reverse the image#s:reverse [on/off]#d:Reverse (or unreverse) the image of the current view. By default Aladin loads images with the reverse mode activated.\n \nIn case of @RGB image, the produced image will take the complementary colors.\n \nThis command is not available for @blink planes.
Help.flipflop	#n:_flipflop_ - vertical or horizontal mirroring#s:@[name=] flipflop [x|v] [V|H|VH]#d:Apply a vertical or horizontal mirroring of the specified image. The astrometrical solution is adapted accordingly.#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:flipflop H#e:foo=flipflop DSS1* VH#g:@copy, @mosaic, @crop
Help.mv	#n:_mv_ - move planes or views#s:mv x1 x2            - for stack manipulation#s:mv v1 v2            - for multiview manipulation#s:mv x1 [x2...] name  - for folder manipulation#d:The "mv" command behaviour depends of the nature of its parameters.\n \nIf the parameters describe two planes (x1 and x2), Aladin will move x1 plane behind the x2 plane in the Aladin stack.\n \nIf the parameters describes two views (v1 and v2) in multiview mode, Aladin will move the view v1 to the v2 place. The v2 view place will be overiden by v1 even if v2 was not empty.\n \nIf the parameters describe planes and the last parameter describes a folder, the planes will be move into the folder.#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@md, @cview
Help.select	#n:_select_ - select views and/or planes#s:1. select x1|v1 [x2|v2] ...#s:2. select [x|v] frame=nn#s:3. select -tag#d:1. Select planes or views by their identifier in order to apply a function to them (see also section)\nA plane identifier can be the number of the plane in the Aladin stack (the bottom one is 1). It can be also the label of the plane, allowing use of the wildcard "*". In this case, the first plane matching the identifier will be taken into account.\n In multiview mode, you may select a view by its coordinates: a letter for the column and a digit for the line, (ex: B2).\nIf a plane containing catalog sources is selected, its sources will be selected also.\n \n2. Select a particular frame for a cube.\n \n3. Select sources previously tagged.#e:select DSS1.V.SERC#e:select A1 A3 C2 1 3 4 DSS1*#e:select (unselect the previous selection)#e:select frame=10#e:select -tag#g:@cview, @tag, @ccate, @thumbnail, @browse
Help.browse	#n:_browse_ - browse the selected sources#s:1. browse#s:2. browse x#d:Browse the selected sources by zooming on the first one, and if required, load a default survey background. If a catalog plane is designed, the sources of the catalog is first selected, and browsed.#e:browse#e:browse CDS/Simbad#g:@select, @thumbnail
Help.tag  #n:_tag_ - tag all selected sources#s:tag#d:This command tags all current selected sources (the sources shown in the measurement frame). \n \nWhen a tagged catalog source is selected, it is displayed with a dedicated magenta color and its associated measurements shown a validated checkbox at the beginning of the line.\n \nUsed with the @search, @select -tag and @createplane commands, it provides a flexible method for generating catalog samples.#e:search Star\ntag\nsearch UV\ntag\nselect -tag\nccate#g:@untag, @search, @select, @ccate
Help.untag  #n:_untag_ - untag all tagged sources#s:tag#d:This command removes all tags previously set on sources via the @tag command (corresponding to the checkbox in source measurement line).#g:@tag, @select
Help.hide	#n:_hide_ - hide planes#s:hide [x1] [x2..]#d:Hide the specified planes (or the selected planes if there is no parameter).#e:hide DSS1.V.SERC#e:hide  (hide the selected planes):#e:hide 1 2 DSS2*#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#g:@show, @select
Help.show	#n:_show_ - show planes#s:show [x1] [x2..]#d:Show the specified planes (or the selected planes if there is no parameter).\n \nIf there is no view of a specified plane, a view will be created automatically. Also, if there is an existing view of the plane but it is not visible (outside the scroll panel), the view scroll bar will be automatically adapted to show it.#e:show DSS1.V.SERC#e:hide  (hide the selected planes):#e:hide 1 2 DSS2*#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#g:@hide, @select
Help.collapse	#n:_collapse_ - collapse folders#s:collapse [FolderName1] [FolderName2...] #d:Collapse the specified folders in the Aladin stack. Without FolderName, the current selected folder is collapsed.#e:collapse FoldA "Folder 1"#g:@expand, @md, @hide, @show, @mv, @rm
Help.expand	#n:_expand_ - expand folders#s:expand [FolderName1] [FolderName2...] #d:Expand the specified folders in the Aladin stack. Without FolderName, the current selected folder is expanded.#e:expand FoldA "Folder 1"#g:@collapse, @md, @hide, @show, @mv, @rm
Help.md	#n:_md_ - create a folder#s:md [-localscope] [name]#d:Create a folder on the top of the Aladin stack. The name can be omitted, in this case it will be automatically created following this syntax: "Fold~nn".\n \nThe -localscope parameter means that the planes in the folder, and only these planes, can be projected on images in the same folder (useful in multiview mode only).\n \nYou can move planes into a folder with the @mv command.#e:md M1-folder#g:@mv, @rm, @hide, @show
Help.cm	#n:_cm_ - set the color map and/or the cut parameters#s:cm [x1|v1 ...] [colorMap | cutParams ...]#d:Modify the colormap and/or the pixel cut parameters of the specified images.\n \nThe color maps are:\n   .gray: 256 gray levels (default color map)\n   .BB: 256 orange levels (useful to improve contrast impression)\n   .A: equal color areas\n   .stern: helping for the distinction of hight pixel values\n   .rainbow: RAINBOW color map from IDL\n   .eosb: Eos B color map from IDL\n   .fire: Fire color map from ImageJ\n \nThe cut parameters are:\n   log|sqrt|linear|pow2: transfer function\n   reverse|noreverse: video mode\n   autocut|noautocut:autocut apply or not\n   localcut:autocut based on the reticle position only\n   min..max|all: original pixel range or all pixels.#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:cm stern#e:cm DSS2* log#e:cm A1 B1 noreverse log 10..100 autocut
Help.rm	#n:_rm_ - delete planes or views#s:rm [x1] [x2..]      - for stack manipulation#s:rm [v1] [v2..]      - for multiview manipulation#s:rm name             - for folder manipulation#s:rm -ROI|-all          - for specifical usage#d:The "rm" command behaviour depends of the nature of its parameters.\n \nIf the parameters describe planes (x1...), Aladin will remove these planes in the Aladin stack and all the associated views.\n \nIf the parameters describe views (v1...), Aladin will remove these views.\n \nIf the parameter is the "-ROI" reserved keyword, Aladin will remove all ROI views (see @thumbnail ). The "-all" parameter will remove all planes and all views.#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@get, @cview, @thumbnail
Help.+	#n:_+_ Image addition#s:@[name=] [x1] + x2#s:@[name=] [x1] + value#d:The "+" command allows you to add two images or one image and a specifical value. The addition will be done pixel per pixel. The resulting image will be coded in Float 32 bits.\n \nIf the images do not have the same astrometrical solution, Aladin will resample the second image in the astrometrical solution of the first one (bilinear method) before adding the pixels.\n \nIf the first operand is omitted, Aladin assumes the first operand is the current image.#t:This command can be prefixed by "PlaneName=" meaning that the result will be saved in this specifical plane. If this plane is already existing, it will be overwritten by the result.\n #t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#e:DSS1.ESO.R + DSS2.SERC.J#e:foo = \@1 + 100#e:+ 2MASS.J#g:@-, @*, @/, @norm, @conv, @bitpix
Help.-	#n:_-_ Image subtraction#s:@[name=] [x1] - x2#s:@[name=] [x1] - value#d:The "-" command allows you to subtract two images or one image and a specifical value. The subtraction will be done pixel per pixel. The resulting image will be coded in Float 32 bits.\n \nIf the images do not have the same astrometrical solution, Aladin will resample the second image in the astrometrical solution of the first one (bilinear method) before subtracting the pixels.\n \nIf the first operand is omitted, Aladin assumes the first operand is the current image.#t:This command can be prefixed by "PlaneName=" meaning that the result will be saved in this specifical plane. If this plane is already existing, it will be overwritten by the result.\n #t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#e:DSS1.ESO.R - DSS2.SERC.J#e:foo = \@1 - 100#e:- 2MASS.J#g:@+, @*, @/, @norm, @conv, @bitpix
Help.*	#n:_*_ Image multiplication#s:@[name=] [x1] * x2#s:@[name=] [x1] * value#d:The "*" command allows you to multiply two images or one image and a specifical value. The multiplication will be done pixel per pixel. The resulting image will be coded in Float 32 bits.\n \nIf the images do not have the same astrometrical solution, Aladin will resample the second image in the astrometrical solution of the first one (bilinear method) before multiplying the pixels.\n \nIf the first operand is omitted, Aladin assumes the first operand is the current image.#t:This command can be prefixed by "PlaneName=" meaning that the result will be saved in this specifical plane. If this plane is already existing, it will be overwritten by the result.\n #t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#e:DSS1.ESO.R * DSS2.SERC.J#e:foo = \@1 * 100#e:* 2MASS.J#g:@+, @-, @/, @norm, @conv, @bitpix
Help./	#n:_/_ Image division#s:@[name=] [x1] / x2#s:@[name=] [x1] / value#d:The "/" command allows you to divide two images or one image and a specifical value. The division will be done pixel per pixel. The resulting image will be coded in Float 32 bits.\n \nIf the images do not have the same astrometrical solution, Aladin will resample the second image in the astrometrical solution of the first one (bilinear method) before dividing the pixels.\n \nIf the first operand is omitted, Aladin assumes the first operand is the current image.#t:This command can be prefixed by "PlaneName=" meaning that the result will be saved in this specifical plane. If this plane is already existing, it will be overwritten by the result.\n #t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#e:DSS1.ESO.R + DSS2.SERC.J#e:foo = \@1 + 100#e:+ 2MASS.J#g:@+, @-, @*, @norm, @conv, @bitpix
Help.norm	#n:_norm_ - Image pixel normalisation#s:@[name=] norm [-cut] [x]#d:The "norm" command normalizes the image pixels between 0 and 1 (float 32bits format). With the "-cut" parameter, the normalisation takes into account the min and max pixel values used by the current pixel mapping (see @cm ), otherwise all original pixel range will be considered.\n \nIf the image designation is omitted, Aladin will work on the current image.#t:This command can be prefixed by "PlaneName=" meaning that the result will be saved in this specifical plane. If this plane is already existing, it will be overwritten by the result.\n #t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#e:norm#e:norm DSS1.SERC.J#e:foo = norm -cut \@1#g:@+, @-, @*, @/, @conv, @bitpix
Help.conv	#n:_conv_ - Image pixel convolution#s:@[name=] conv [x] kernelName#s:@[name=] conv [x] gauss({fwhm|sigma}=angle[,radius=nn])#s:@[name=] conv [x] n00 n01 n02... n10 n11 n12...#d:The "conv" command applies a convolution on the specified image.\nThe kernel can be designated either by its name, or a gaussian filter, or a specifical matrix. See @kernel command for details.\n \nIf the image designation is omitted, Aladin will work on the current image.#t:This command can be prefixed by "PlaneName=" meaning that the result will be saved in this specifical plane. If this plane is already existing, it will be overwritten by the result.\n #t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#e:conv Gauss2.5#e:foo = conv \@1 Mex5#g:@kernel, @+, @-, @*, @/, @norm, @bitpix
Help.bitpix	#n:_bitpix_ - Image pixel re-encoding#s:@[name=] bitpix [-cut] [x] BitpixCode#d:The "bitpix" command re-encodes image pixel values.\nThe target pixel format follows the FITS conventions: -64: double, -32: float, 64: long, 32: integer, 16: short, 8:byte\nWith the -cut option, the visible range of pixel values is extended for the best in the target encoding space, otherwise, a simple "casting" is operated. In this last case, too large values (resp. too small values) are forced to the target range limits.\nIf the image designation is omitted, Aladin will work on the current image.#t:This command can be prefixed by "PlaneName=" meaning that the result will be saved in this specifical plane. If this plane is already existing, it will be overwritten by the result.\n #t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).#e:bitpix -32#e:imgTgt = bitpix -cut imgSrc 16#g:@conv, @+, @-, @*, @/, @norm
Help.kernel	#n:_kernel_ - Convolution kernel definition#s:kernel name=n00 n01 n02... n10 n11 n12...#s:kernel name=gauss({fwhm|sigma}=angle[,radius=nn])#s:kernel [mask]#d:The "kernel" command allows you to define new convolution kernels which can be used on images via the @conv command. The matrix can be fully provided (line after line), or defined by a gaussian filter. In this case, it is possible to specify the FWHM or the sigma (by default in arcmin but any angle unit can be added); The matrix radius can also be specified. If it is omitted, Aladin will find it automatically at 3 x sigma. A name must precede the matrix definition.\n \nWithout matrix definition, kernel command displays the list of already available kernels or, if a specifical kernel name is given, the associated matrix.#t:Aladin has a list of predefined kernels.#e:kernel myShift=1 0 0 0 0 0 0 0 0#e:kernel mygauss=gauss(fwhm=30')#e:kernel mygauss*#g:@conv, @+, @-, @*, @/, @norm
Help.reset	#n:_reset_ - reset Aladin#s:reset#d:Reset Aladin by removing all views and all planes. Restore one view mode and clean the memory.#g:@rm
Help.copy	#n:_copy_ - copy planes or views#s:1. copy [x] [foo]#s:2. copy v1 v2#d:1. Allow one to create a copy of the plane x (the selected one by default) to a new plane called "foo". Another syntax for the same command can be "foo=x" (see @[name=] for details).\n #d:2. Allow one to create a copy of the view v1 to v2 place (see multiview mode: @mview). Notice that each view can have is own zoom factor but still share the same image properties notably the colormap.\n \nCopying a plane rather than a view allows one to modify the images independently (colormap, cropping...) but use more memory.#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:copy "DSS2.J.SERC" foo#e:copy inOtherPlane#e:copy A2 C3#g:@cview, @mv, @cm, @crop, @zoom
Help.rgb	#n:_RGB_ - create a RGB image#s:@[name=] RGB [x1|v1 x2|v2 x3|v3]#d:Create a colored composed image from three images. The images can be specified by their plane or by their view (in multiview mode). The first image provides the Red component, the second image provides the Green component and the last image the Blue component. Each image is resampled according to the astrometrical solution of the first image.#e:RGB \@2 \@3 4#e:RGB DSS1* DSS2* MAMA*#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@RGBdiff, @blink, @resamp, @mosaic
Help.cmoc	#n:_cmoc_ - create a MOC (space, time, or space-time coverage)#s:@[name=] cmoc [-order=o] [-pixelCut=min/max] [x1|v1 ...]#s:@[name=] cmoc [-order=o] [-radius=angle|-fov] [x1|v1 ...]#s:@[name=] cmoc [-order=o] [x1 ...]#s:@[name=] cmoc -threeshold=0.x [x|v]#s:@[name=] cmoc AsciiMOC#s:@[name=] cmoc -op [x1|v1 ...]#d:These syntaxes create a MOC respectively from images, catalogs, polygons or circles, probability maps and ASCII MOC string. By default the result is a space MOC. The last syntax allows to combine MOCs (-union, -inter, -sub, -diff, -compl).\n \n  .o specifies the moc order (11 by default => 1.718').\n  .min/max specifies a range of pixel values (NaN as infinity).\n  .angle specifies a radius around catalog sources (default arcsec).\n  .-fov uses Field of Views (s_region) associated to each source\n  .threeshold specifies a cumulative probability threeshold (<=1)#e:cmoc -order=13 -pixelcut="2 NaN" DSS2#e:cmoc -order=15 -radius=1' cat1 cat2#e:cmoc 3/1-4 4/5-32 36#e:cmoc -inter moc1 moc2 moc3#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@export, @load#g:java -jar Aladin.jar -mocgen -h (batch MOC generator)\n \n@rescmoc, @moreoncmoc for time dimension...
Help.moreoncmoc	#n:_cmoc_ - cmoc time support#s:@[name=] cmoc -time [-order=o] [-duration=t] [x1|v1 ...]#s:@[name=] cmoc -spacetime [-order=so/to] ... [x1|v1 ...]#s:@[name=] cmoc [-order=o] [-timeRange=date1/date2] [x1 ...]#d:The cmoc command is also able to generate and manipulate time coverages (TMOC) and/or space-time coverages (STMOC). The time dimension can be visualized in dedicated time view (see @cview -plot). Most of regular cmoc parameters may be combine with TMOC and STMOC specifical parameters.\n \n  -time create a time MOC\n  -spacetime create a space time MOC\n \n  .o specifies the time moc order (11 by default => 19h5mn20s).\n     spaceOrder/timeOrder syntax for space time MOC.\n  .duration in seconde\n  .date1/date2 time range (ISO syntax, see examples)#e:cmoc -time -order=15 -duration=300 cat1 cat2#e:cmoc -spacetime -order=10/12 -duration=300 -fov cats#e:cmoc -timerange=2020-01-01/2020-12-31T23:59 stmoc1#e:cmoc -spacetime -o=/13 -timeRange=2001-05-01/2001-05-31 smoc#g:@cview -plot
Help.rescmoc	#n:_cmoc_ - resolution tables\n \n \nSpace Moc resolution table:\n \n    0:58.63        8:13.74'       16:3.221"       24:12.58mas  \n    1:29.32        9:6.871'       17:1.61"        25:6.291mas  \n    2:14.66       10:3.435'       18:805.2mas     26:3.145mas  \n    3:7.329       11:1.718'       19:402.6mas     27:1.573mas  \n    4:3.665       12:51.53"       20:201.3mas     28:786.3as  \n    5:1.832       13:25.77"       21:100.6mas     29:393.2as  \n    6:54.97'       14:12.88"       22:50.32mas  \n    7:27.48'       15:6.442"       23:25.16mas  \n\n \nTime Moc resolution table:\n \n   0:73067y 276d  16:1y 41d       32:8m 56s       48:8ms 192s  \n   1:36533y 320d  17:203d 14h     33:4m 28s       49:4ms 96s   \n   2:18266y 342d  18:101d 19h     34:2m 14s       50:2ms 48s   \n   3:9133y 171d   19:50d 21h      35:1m 7s        51:1ms 24s   \n   4:4566y 268d   20:25d 10h      36:33s 554ms    52:512s      \n   5:2283y 134d   21:12d 17h      37:16s 777ms    53:256s      \n   6:1141y 249d   22:6d 8h        38:8s 388ms     54:128s      \n   7:570y 307d    23:3d 4h        39:4s 194ms     55:64s       \n   8:285y 153d    24:1d 14h       40:2s 97ms      56:32s       \n   9:142y 259d    25:19h 5m       41:1s 48ms      57:16s       \n  10:71y 129d     26:9h 32m       42:524ms 288s  58:8s        \n  11:35y 247d     27:4h 46m       43:262ms 144s  59:4s        \n  12:17y 306d     28:2h 23m       44:131ms 72s   60:2s        \n  13:8y 335d      29:1h 11m       45:65ms 536s   61:1s        \n  14:4y 167d      30:35m 47s      46:32ms 768s \n  15:2y 83d       31:17m 53s      47:16ms 384s \n
Help.rgbdiff	#n:_RGBdiff_ - create a RGB image with the difference of two images#s:@[name=] RGBdiff [x1|v1 x2|v2]#d:Create a colored composed image from the subtraction of two images. The images can be specified by their plane or by their view (in multiview mode). The resulting pixels greater than zero are displayed in red color, the other pixels are displayed in green color. The second image is resampled according to the astrometrical solution of the first image.#e:RGBdiff \@2 \@3#e:RGBdiff DSS1* DSS2*#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@RGB, @blink, @resamp, @mosaic
Help.blink	#n:_blink_ - create a blink sequence of images#s:@[name=] blink [x1|v1] [x2|v2...]#d:Create a blink sequence of several images (at least 2 images). The images can be specified by their plane or by their view (in multiview mode). Each image is resampled according to the astrometrical solution of the first image.#e:blink 2 3 4 5#e:blink DSS1* DSS2*#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@RGB, @resamp, @mosaic
Help.mosaic	#n:_mosaic_ - create a mosaic image#s:@[name=] mosaic [x1|v1] [x2|v2...]#d:Create a mosaic image of several images. The images can be specified by their plane or by their view (in multiview mode). Each image is resampled according to the astrometrical solution of the first image (closest pixel algorithm). The overlaying pixels will be averaged. The mosaic uses the 8 bits pixels of each image (take into account the cut level process). It is not possible to create mosaics from the original pixels. #e:mosaic \@2 \@3 \@4 \@5#e:mosaic DSS1* DSS2*#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@blink, @RGB, @resamp, @crop
Help.crop	#n:_crop_ - Image cropping#s:@[name=] crop [x|v] [[X,Y] WxH]#d:Crop the specified image to the area defined by the X,Y,W,H parameters, where X,Y determines the up-left corner and W,H determines the size. If X,Y is omitted, the area is centered on the reticle location. If both X,Y and W,H are omitted, the current zoom area is used. If the area is partially outside the image, the area is automatically adjust to the intersection.\n \nThe crop applied on an "allsky" plane :\n  - is only possible if this plane is activated and visible;\n  -  in case of true pixel display mode (FITS tiles) : applied a full bilinear resample on the best possible resolution of the survey => use it carefully in case of large area. The result is a Fits image;\n  - otherwise, applied a simple dump of view. The result is a JPEG image#e:crop DSS2.J.SERC 100,50 300x200#e:crop 300x400#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@copy, @mosaic, @flipflop
Help.grey	#n:_grey_ - color image conversion#s:grey#d:Convert the current RGB image selected in the stack into a monochromatic image (grey levels)#e:grey#g:@cm, @RGB
Help.resamp	#n:_resamp_ - create a resampled image#s:@[name=] resamp x1|v1 x2|v2 [8|Full] [Closest|Bilinear]#d:Resample a image according to the astrometrical solution of another image.\n \nAvailable parameters:\n   -8: only on visual pixels (8 bits depth) - default\n   -(F)ull:on the real pixels if they are avaiable\n   -(C)losest: Closest pixel algorithm (the fastest)\n   -(B)ilinear: Bilinear interpolation algorithm (better) - default#e:resamp 2 3#e:resamp DSS1* MAMA*#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#g:@RGB, @blink
Help.grid	#n:_grid_ - coordinate grid management#s:grid [on|off|hpx]#d:Switch the coordinate grid on or off. The keyword "hpx" (or "healpix") is used for displaying a HEALPix grid.#e:grid on#g:@setconf overlays=..., @reticle, @overlay
Help.reticle	#n:_reticle_ - reticle management#s:reticle [on|off|large]#d:Switch on or off the reticle designating the last click position.\nThe reticle is displayed as a large magenta colored cross or two magenta (vertical & horizontal) lines. In this last case, you have to specify the "large" parameter instead of "on".#t:- An astronomical object or sexagesimal J2000 coordinates simply written instead of an Aladin script command will automatically move the target (and the reticle) to the corresponding position#g:@lock, @setconf overlays=..., @grid, @overlay
Help.overlay	#n:_overlay_ - Overlay information management#s:overlay [on/off]#d:Switch on or off the overlay information on the views (scale, plane name, North direction, field size).#g:@setconf overlays=..., @grid, @reticle
Help.draw	#n:_draw_ - graphical overlay commands:draw fct(param)#s:draw [color] fct(param...)\ndraw newtool[(name)] or draw newfov(xcenter,ycenter[,name])\ndraw STC ...\ndraw MOC ...#d:Allows one to manually add graphical overlays on views. There are several graphical functions available:\n  .string(x,y,text)             .tag(x,y[,label,dist,angle,type,ftSize])\n  .line(x1,y1,x2,y2,...[,txt])  .polygon(x1,y1,x2,y2,...[,txt])\n  .vector(x,y,w,angle)          .dist(x1,y1,x2,y2)\n  .box(x,y,dx,dy[,angle,label]) .ellipse(x,y,semiMA,semiMI,angle)\n  .circle(x,y,r)                .phot(x,y,r[,order|max])\n  .arc(x,y,r,PA,angle)          .pickle(x,y,r1,r2,PA,angle)\nThe coordinates must be expressed in the current coordinate frame. It can be image XY coordinates (use @setconf frame=XY)\nBy default, Aladin puts the new object in the last drawing plane in the stack. It is possible to create manually a new one by the "draw newtool(name)" or "drawfov(x,y,name)" commands.#t:-The parameter separator can be the comma or the space. In case of coordinates use the colon to group the subfields or quote them\n-The default angle unit is degree\n-The color parameter is specified as colorName or rgb(n,n,n)\n- The tag types are: reticle, bigreticle, smallcircle, circle, bigcircle, arrow, bigarrow, nopole\n-DS9 region commands or STC-S regions are automatically translated in the corresponding "draw" commands (ex: STC Circle ICRS 147.6 69.9 0.4).\n-MOC is always created in a separated plane (ex: draw MOC 3/2-30 4/134,136)#e:draw string(300,200,"my favourite galaxy")#e:draw rgb(100,34,89) tag(10:12:13,+2:3:4,"Big galaxy",100,30,circle,22)#e:draw red circle("1 2 3" "+4 5 6" 3arcmin)
Help.status	#n:_status_ - Aladin stack/views status#s:status [{stack|views|x1 [x2...]}]#d:display the stack status, or view status or the status of specified planes or views on the standard output (all planes and views by default).#e:status\n \nPlaneID Simbad\nPlaneNb 2\nType    Catalog\nStatus  shown \nUrl     http://simbad.u-strasbg.fr/cgi-bin/simbad-xml.pl?Ident=m1\nTarget  05:34:31.97 +22:00:52.1\nNbObj   43\nShape   dot\nColor   blue\n \nViewID  A1\nCentre  05:34:31.61 +22:00:52.1\nSize    28.06' x 28.0'\nZoom    1x\nProj    [Simbad] TANGENTIAL\nStatus  selected#g:@set
Help.hist	#n:_hist_ - history#s:hist [n]#d:Display the script command history in the Aladin console and on the standard output. By default, the last 10 commands are displayed.#e:hist 20#g:@status
Help.info	#n:_info_ - message status#s:info msg#d:Print a message in the status window (between the main frame and the measurement frame). If the @demo mode is activated, the message will be displayed in a separated window#g:demo
Help.help	#n:_help_ - in line help#s:help [cmd|all|allhtml|off]#d:display this help for each command and a resume of all available commands if there is no parameter.\n \nThe "off" parameter allows one to display the current view again.\n \nThe "all" parameter allows one to print on the console help about all Aladin script commands. The same thing is done in HTML with "allhtml" parameter.
Help.pause	#n:_pause_ - script pause#s:pause [nn.nnn]#d:wait nn.nnn seconds, 1 by default. Very useful for demonstration...
Help.sync	#n:_sync_ - manual plane synchronization#s:sync#d:Wait explicitely until all planes are ready (corresponding to a "not blinking status plane").\n \nBy default Aladin is running in auto sync mode meaning that script commands requiring previous results will automatically wait until all planes in the stack are ready. However, this @sync command can force a synchronisation at any time or if the user has removed the auto sync mode via the @setconf syncproperty.#e:setconf sync=off; A=get ESO M1; sync; A = A/2#g:@setconf
#Help.timeout	#n:_timeout_ - timeout control#s:timeout nn|off#d:This command is related to the @get command. By default a get command will be stopped after 15mn if there is no activity from the remote server. With the timeout command you may increase or decrease this limit, or suppress it at all together.#e:timeout 30#e:timeout off#g:@get
Help.mem	#n:_mem_ - memory status#s:mem#d:Display the java memory used (after a garbage collector).
Help.quit	#n:_quit_ - end of Aladin session#s:quit#d:Stop Aladin
Help.mview	#n:_mview_ - multiview controler#s:mview [1|2|4|9|16] [n]#d:Specify the number of simultaneous views and the number of the first one (the first is 1)#e:mview 9#e:mview 4 3#g:@cview, @show
Help.cview	#n:_cview_ - creation of view#s:cview [[x] v]#s:cview -plot x(columnName,columnName) [v]#d:This command can only be used in multiview mode. It allows one to manually create a view at the position "v" of the Aladin plane stack "x".\n \nThe "-plot" param allows you to create a scatter plot instead of a sky view. It is only relevant for catalogue planes. if a scatter plot is already existing in the specified view, Aladin will add the new catalogue to the existing plot.#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:cview DSS1.V.SERC C3#e:cview 2   (use a default view place for the plane number 2)#e:cview -plot Simbad(PMRA,PMDEC)#g:@mview, @mv, @copy, @rm
Help.match	#n:_match_ - view "matching" mode#s:match [-scale] [v|x]#s:match off#d:Within the multiview mode, it is possible to match the scale and the orientation, of different images sampling the same region in the sky. Matching only scales does not affect pixels, it only select automatically the closest centre and zoom factor in order to visualise the same region of the sky. This is not the case when matching both scales and orientation since it re-projects images using the location of the 4 corners of the image: images are identical but pixels have been put out of shape.\n \nThe reference of the matching can be explicitely specified (the current select view is the default)#t:"x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1).\n"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:match#e:match DSS1#e:match -scale B1#e:match off#g:@mview, @select
Help.lock	#n:_lock_ - lock the view#s:lock [v1] [v2...]#d:The "lock" behavior is interesting notably in multiview mode and if the view does not show all the image (depending of the zoom factor and the image size and the Aladin frame size in the screen). In this case, the zoom factor and the central position of a such view are locked until you @unlock it#t:"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:lock A2 C3#g:@unlock, @stick, @unstick, @zoom, @reticle
Help.unlock	#n:_unlock_ - Unlock views from the reticule position#s:unlock [v1] [v2...]#d:The "lock" behavior is interesting notably in multiview mode and if the view does not show all the image (depending of the zoom factor and the image size and the Aladin frame size in the screen). In this case, the zoom factor and the central position of a such view are locked until you @unlock it#t:"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:unlock C1#g:@lock, @stick, @unstick, @zoom, @reticle
Help.stick	#n:_stick_ - view "sticking"#s:stick [v1] [v2...]#d:By default, an Aladin view can be scrolled (according to the current multiview mode). A view may be sticked to keep it in the same place even if you scroll the view panels.\n \nThis funtion is very useful in multiview mode in order to easely select a set of views amongst many views (typically generated by the ROI extraction mechanism), by moving the interesting view into a "sticked" view#t:"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:stick A1 A2 A3#g:@unstick, @lock, @unlock, @cview, @mv, @thumbnail
Help.unstick	#n:_unstick_ - view "unsticking"#s:unstick [v1] [v2...]#d:By default, an Aladin view can be scrolled (according to the current multiview mode). You can stick a view to keep it in the same place even if you scroll the view panels.\n See @stick command.#t:"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:unstick B2#e:unstick    (unstick all views)#g:@stick, @lock, @unlock, @cview, @mv, @thumbnail
Help.northup	#n:_northup_ - view north oriented#s:northup [v1] [v2...]#d:By default, an Aladin view is drawn according to the astrometrical solution of the reference plane (generally the background image). This function will force the view to draw North up, East left.#t:"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:northup#g:@unnorthup, @cview, @grid
Help.unnorthup	#n:_unnorthup_ - view default oriented#s:unnorthup [v1] [v2...]#d:Re-use the default orientation of the view according to the astrometrical solution of the reference plane (generally the background image).#t:"v" is the grid coordinate of a view with a letter for the column and a digit for the line, ex: B2#e:unnorthup B2#e:unnorthup#g:@northup, @cview
Help.search	#n:_search_ - Search and select specifical catalog sources#s:search [-|+]expression#s:search {-|+}#d:The search command selects all sources matching the parameter expression. The search is done amongst all sources in the stack catalog planes.\n \nWith the prefix '+', the matched sources will be appended to a previous selection, with the prefix '-', the matched sources will be removed of the previous selection\n \nThe expression can be\n   .a keyword\n   .a column name followed by a boolean expression (ex:Type=Star)\n   .a column name embedeed in abs. characters followed by a boolean expression (ex: |PM|>10)\n \n The + or - parameter without any expression moves the reticle on the next source (resp. the previous source) of the previous search.\nWith a hight zoom value, it provides a powerful tool for browsing quickly a list of sources.#e:search |Mag|>=10#e:search -OTYP*!=UV#e:search +#g:@zoom, @select, @tag, @ccate
#Help.cplane	#n:_cplane_ - source plane creation#s:cplane [name]#d:Create a new catalog plane in the Aladin stack with the current selected sources.\n \nThis command is useful to extract a set of objets after applying a @filter, or to merge two catalog planes together (select x1 x2; cplane).#t:Notice that the @select command on a catalog plane also selects its sources. The typical sequence could be:\n   gsc = get Vizier(GSC2.2) HD1\n   filter mag { $[phot.mag*]<16.5 || $[phot.mag*]>17 { hide } }\n   filter mag on\n   select gsc\n   cplane MySelection#g:@select, @get, @export
Help.ccat	#n:_ccat_ - source plane creation#s:@[name=] ccat [-uniq] [x1 x2 ...]#s:@[name=] ccat [-out] xmoc [x1 ...]#d:Create a new catalog plane in the stack with the sources of the specified planes or, by default, the current selected sources. A MOC plane can be specified for filtering the sources.\n \nThe -uniq parameter will force to generate an unique table, even if the source have various measurement columns. The -out parameter changes the default MOC filtering behaviour for keeping the sources outside the MOC rather than inside the MOC.\n \nThis command is notably useful to merge two catalog planes together (ccat x1 x2) or to extract a set of objets after applying a @filter.#t:Notice that the @select command on a catalog plane also selects its sources. The typical sequence could be:\n   gsc = get Vizier(GSC2.2) HD1\n   filter mag { $[phot.mag*]<16.5 || $[phot.mag*]>17 { hide } }\n   filter mag on\n   select gsc\n   MySelection=ccat#g:@select, @get, , @cmoc, @export
Help.thumbnail	#n:_thumbnail_ - Thumbnail view generator#s:thumbnail [npixels|radius]#d:Allows one to automatically create zoomed views around the current selected objects/sources for the selected images (one or more). In this way, it is possible to rapidly browse and/or compare a large set of objects.\nThe size of the zoom views can be determined either in pixels (default 40) or in angular angle (do not forget to mention the unit => , " or '). The generated views are automatically locked: you will not be able to modify the position and the zoom factor of them.#t:The typical usage should be\n   mview 9\n   get hips(P/DSS2/color)\n   get VizieRX(gliese)\n   filter mag{  $[phot.mag*]>8 && $[phot.mag*]<13 { draw } }\n   filter on\n   thumbnail 5"#e:thumbnail#g:@select, @rm Lock
#Help.rename	#n:_rename_ - name or rename plane#s:rename [x] name#d:Allow one to name or rename the plane "x" (or by default, the first selected plane).\n \nIf the name is already used in the stack, Aladin will automatically append an extension "~n".#t: - The @get command automatically sets a name to the resulting plane. The usage of "rename" command allows one to override this default name.#t: - "x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1)#g:@get, @select
Help.set	#n:_set_ - modify a plane property#s:set [x1] [x2...] prop=value#s:set x/component prop=value#s:set x FITS:keyword=value#d:Allow one to modify a propertie of the planes specified by "x" (or by default, the selected planes).The "prop" is a keyword describing a plane propertie. The keyword list for a given type of plane can be obtained by the status script command on this plane.\n \nIf the propertie is concerning only a component of the plane (for instance a sub-FoV of a Field plane), the plane designation has to be suffixed by the component name (with / separator).\nThe dedicated "FITS:" value prefix allows one to modify directly the FITS header associated to a plane, and by this way it is possible to modify the WCS keywords and the associated astrometrical calibration#t: - Notice that the "value" can not contain the character "=".#t: - "x" can be the plane label (allowing use of "*" wildcard) or the plane number in the stack prefixed by \@ (the bottom one is \@1)#e:set Sim* PlaneID=MyPlane #e:set Simbad filter=All objects#e:set HST/FGS2 Status=hide#e:set DSS1* FITS:CRPIX1=400#g:@status, @setconf
Help.setconf	#n:_setconf_ - modify a session property#s:setconf prop=value#d:Allow one to modify a configuration propertie.\nThe available properties are:\n \n.frame      coordinate frame (ICRS|ICRSd|J2000|J2000d|B1950|B1950d\n            |Ecliptic|Gal|SGAL|XY image|XY linear);\n.bookmarks  function name list\n            (comma separated possibly precedeed by + or -);\n.overlays   overlay list (scale,label,size,NE,grid,reticle,target,pixel,colormap)\n            (comma separated possibly precedeed by + or -);\n.colormap   pixel mapping (autocut|noautocut reverse|noreverse)\n            gray|BB|linear|stern|rainbow|eosb|fire\n            log|sqrt|linear|pow2);\n.dedicatedfilter dedicated filters (on|off);\n.dir        default directory;\n.gridFontSize,infoFontSize           Font size (n,+n,-n)\n.gridcolor,gridcolorRA,gridcolorDEC  Grid color control\n.labelcolor,infocolor,infoborder (on|off)    Overlay info control\n.sync       auto sync mode (on|off)\n.timeout    plane loading timeout (in mn|off)#e:setconf Dir=/home/mydir#e:setconf frame=Gal#e:setconf bookmarks=DSS,Simbad,NED#e:setconf CSV=:#e:setconf colormap=autocut BB noreverse#e:setconf overlays=-NE#e:setconf labelcolor=RGB(160,45,15)#g:@set, @sync, @function, @call, @list, @overlay
Help.macro	#n:_macro_ - execute a macro#s:macro scriptFile paramFile#d:Allow one to launch a macro via a script command (see manual for macro details). The scriptfile contains the list of commands, one per line. Use $1, $2 as parameters. The paramFile contains the list of parameters for each macro execution. The parameters for the first execution are provided by the first line, the parameters must be separated by "TAB" character. The second line contains the list of parameters for the second macro execution, etc.\n \nscriptFile and paramFile can be pathfile or url (remote access via web)#e:macro myscript.ajs myparams.txt#e:macro myscript.ajs http://myserver.org/getParamFor?M1
Help.function	#n:_function_ - script function definition#s:function name[($param,...)] {\n   code...\n}#d:For defining a script function callable by the @call command. The function name can be followed by a parameter list (syntax: $xxxx,$yyy,...) which will be subsituted by the call(xxx,yyy,...) values.\n \nVia the @setconf bookmarks=[+|-]functionName,... any function can be used for defining a bookmark appearing in the Aladin bookmark bar. #t:The dedicated parameter names $TARGET and $RADIUS will be substituted by the current view area parameters if these values are not specified in the @call command.#e:function data($TARGET) { get simbad $TARGET;get NED $TARGET }#g:@call, @list, @setconf
Help.call	#n:_call_ - script function call#s:call [-batch] fonctionName[(param,...)]#d:For calling a script function previously defined via the @function command.\n \nThe -batch flag insures that the list of function script commands will be executed sequentially, and that, without the autosync @sync mechanism activated for this function. By this way, the function can be called without waiting the end of another script command not yet synchronized #e:call data(m1)#e:call -batch browseVizieR#g:@function, @list, @sync, @setconf
Help.list	#n:_list_ - function list and function edition#s:list#s:list functionNameMask#d:Provides the list of defined functions. If a functionNameMask is specified (with possible * and ? wilcards), the matching functions are totally edited#e:list#e:list data#g:@function, @call, @setconf
Help.print	#n:_print_ - print function#s:print#d:Allow one to print the current views. In case of multiview mode, the visible views will be printed on the same page#t:Unfortunately, Java Printer method opens automatically a stupid driver window before printing. So this command CANNOT REALLY BE USED as a "script" command.
Help.demo	#n:_demo_ - demonstration mode#s:demo [on|off|end]#d:Switch on or off the demonstration mode. If the demonstration mode is activated, the script commands will be "demonstrated" by explaining step by step how to obtain the same result with the Aladin graphical interface.\n \nA typical usage:\n   demo on\n   get Aladin(MAMA) galactic center#t:Not all script command have a "demo" mode implemented. In this case, the command is simply executed.
Help.filter	#n:_filter_ - Define and activate a filter#s:filter name {\n  condition1 { draw|hide [color] [action1] }\n  condition2 { draw|hide [color] [action2] }\n   :\n}#s:filter [name] {on|off}#d:A filter is a special plane constraining how the sources of the catalog planes beneath it in the Aladin stack will be displayed.\n \nThe first syntax allows to define a new filter, the second syntax allows switching the specified filter on or off.\n \n Available operators are +,-,*,/,^(power).\nAvailable functions are "abs" (absolute value), "cos" (cosinus), "deg2rad" (degrees to radians), "exp" (exponential), "ln" (natural logarithm), "log" (base 10 logarithm), "rad2deg" (radians to degrees), "sin" (sinus), "tan" (tangent). \n \nThe available actions are: square, cross, rhomb, plus, dot, microdot, circle(param,[min radius size, max radius size]), fillcircle(param,[min radius size, max radius size]), ellipse(semi-major axis,semi-minor axis,pos angle), pm(proper motion RA,proper motion Dec), rainbow(param)\n \n@moreonfilter...
Help.moreonfilter	#n:_filter_ - continuation...\n \nThe column references can be specified by their name: syntax ${name} or by the UCD associated to: syntax $[UCD]. The wildcard "*" can be used both for column name or UCD designation. In the case of multiple matching columns, the first one will be taken into account.#e:filter star { $[CLASS_OBJECT]="Star" { draw } }#e:\nfilter flux {\n   ${flux}>1000000 Jy/s {\n      draw cyan plus\n      draw circle(-$[PHOT*])\n   }\n}#t:Refer to the Filters manual for more details.
Help.addcol	#n:_addcol_ - column generator#s:addcol [plane index or plane name],[new column name],[expr of new col],[unit for new col],[UCD for new col],[nb of decimals to keep]#d:Allow one to generate a new column for a tabular data plane. The new column will appear in red color in the measurement frame.\nThe column references can be specified by their name: syntax ${name} or by the UCD associated to: syntax $[UCD].\nAvailable operators are +,-,*,/,^(power).\nAvailable functions are "abs" (absolute value), "cos" (cosinus), "deg2rad" (degrees to radians), "exp" (exponential), "ln" (natural logarithm), "log" (base 10 logarithm), "rad2deg" (radians to degrees), "sin" (sinus), "tan" (tangent).\nUCD and unit parameters are optional and can be left blank.\n#e:addcol GSC2.2,B-V,${Bmag}-${Vmag},,PHOT_MAG\naddcol 1,flux,10^(0.4*(8.46-${Imag}))
Help.xmatch	#n:_xmatch_ - Cross match tool#s:@[name=] xmatch x1 x2 [max dist in arcsec] [allmatch|bestmatch|nomatch]\nxmatch x1[(RAcol1,DECcol1)] x2[(RAcol2,DECcol2)] ...#d:Allows one to cross match two tabular data planes. The result will be set in a new catalogue plane, including a column with the separation (in arcsec) between the 2 matching sources in arcsec, and all fields of both planes x1 and x2.\n \nThe cross-match is positionnal. x1 contains the reference objects, for which we seek counterparts in x2. One object of x1 is considering match with an object of x2 if they are separated by a distance <="max dist". If the max distance is not set, a default value of 4 arcsec is used.\n \n- In "allmatch" mode, if an object in x1 has several matches in x2, all matches will be kept in the result plane.\n- In "bestmatch" mode, only the closest match will be kept.\n- In "nomatch" mode, we keep only sources of x1 having no match in x2.\nBy default, the "bestmatch" mode is taken into account\n \nCoordinate fields are found according to proper UCDs (pos.eq.ra  and pos.eq.dec for UCD1+, POS_EQ_RA and POS_EQ_DEC for UCD1).\nOptional parameters allow you to specify for each plane which coordinate fields should be used for the cross-match.\nIf nothing is specified, and if proper UCDs are not found, we try in last resort to make a guess on the basis of the field names.\n \n@moreonxmatch...
Help.moreonxmatch	#n:_xmatch_ - continuation...\n \n#t:"x1" and "x2" can be either a plane label (allowing use of "*" wildcard) or a plane number in the Aladin stack (the bottom one is 1).\n \n#e:xmatch 1 2\nxmatch Simbad GSC2.2 10 allmatch\nxmatch 2MASS MyTable(colRA,colDEC) 15\nxmatch T1(RA2000_tab2, DE2000_tab2) T2(RA_tab2, DE_tab2) 10 nomatch
Help.contour	#n:_contour_ - Draw isocontours of the current image#s:@[name=] contour [ nn [nosmooth] [zoom] ]#d:Draw nn isocontours for the current selected image.\nThe result is set in a new plane which can be overlaid on other images of the same field.\n \nnn sets the number of contours to draw. If not defined, 4 contours are plotted by default.\n \nThe parameter nosmooth allows one to switch the smoothing feature off. Smoothing allows a faster computation and reduces the number of control points. It is activated by default.\n \nThe parameter zoom restricts the computation to the current view of the selected image plane. By default, contours are computed over the whole image.
Help.coord	#n:_coord_|_object_ - show a specifical position#s:hh mm ss {+|-}dd mm ss [sys]  - sexagesimal notation#s:dd.dddd  {+|-}dd.dddd [sys]   - decimal notation#s:xxxx                          - astronomical object identifier#d:Set the display position by moving the reticle (large magenta colored cross) on it. The coordinates can be suffixed by a specifical reference system (ICRS, FK5, FK4, GAL, SGAL, ECL), otherwise Aladin assumes the current default reference system (see @setconf frame=...). If the user indicates an astronomical object instead of coordinates, Aladin will automatically query CDS sesame resolver to have the corresponding coordinates.#e: 05 34 31.97 +22 00 52.1#e: 083.63131 +22.01160 SGAL#e: M1#g:@lock, @reticle, @timerange, @setconf
Help.object	#n:_coord_|_object_ - show a specifical position#s:hh mm ss {+|-}dd mm ss [sys]  - sexagesimal notation#s:dd.dddd  {+|-}dd.dddd [sys]   - decimal notation#s:xxxx                          - astronomical object identifier#d:Set the display position by moving the reticle (large magenta colored cross) on it. The coordinates can be suffixed by a specifical reference system (ICRS, FK5, FK4, GAL, SGAL, ECL), otherwise, Aladin assumes the current default reference system (see @setconf frame=...). If the user indicates an astronomical object instead of coordinates, Aladin will automatically query CDS sesame resolver to have the corresponding coordinates.#e: 05 34 31.97 +22 00 52.1#e: 083.63131 +22.01160 SGAL#e: M1#g:@lock, @reticle, @timerange, @setconf
Help.timerange	#n:_timerange_|_time_ - Set the display time range#s:YYYY-MM-DD[THH:MM:SS] YYYY-MM-DD[THH:M:SS] - time range by 2 ISO dates#s:YYYY-MM-DD[THH:M:SS]                      - middle time by an ISO date#d:Set the current display time range, or shift the middle time of the previous time range.\nAll catalog sources with a timestamp field and all time MOC elements outside this time range will be hidden.\n \nThe NaN value is used to reset the limits of the current time range.#e: 1994-01-01 2001-12-31#e: 2019-05-09T10:39:00#e: NaN NaN#g:@coord, @object, @cview
Help.time	#n:_timerange_|_time_ - Set a specifical time range#s:YYYY-MM-DD[THH:M:SS] YYYY-MM-DD[THH:MM:SS] - time range by 2 ISO dates#s:YYYY-MM-DD[THH:M:SS]                      - middle time by an ISO date#d:Set the current display time range, or shift the middle time of the previous time range.\nAll catalog sources with a timestamp field and all time MOC elements outside this time range will be hidden.\n \nThe NaN value is used to reset the limits of the current time range.#e: 1994-01-01 2001-12-31#e: 2019-05-09T10:39:00#e: NaN NaN#g:@coord, @object, @cview
Help.trace	#n:_trace_ - turn on (resp. off) the debug verbose mode#s:trace {1|2|3|off}#d:Aladin supports 3 trace mode levels. The trace messages are displaying in the Aladin console windows and on the standard output, typically the xterm or the window console in which you launched Aladin.
Help.convert	#n:_convert_ - Unit converter#s:convert val unit1 to unit2#d:Unit converter facility. The "val" parameter can be an arithmetic expression or a simple scalar. The more common supported units are Hz, A,m,au,pc,lyr,  deg,rad,sr,mas,arcmin,arcsec,uas,  erg,ev, Pa,bar, g,solMass,geoMass,jovMass, JD,a,m,d ... The full unit list is provided with convert command without any parameter. All multiples and unit compositions are supported. #e:convert 1.3*125km/s to pc/a
Help.=	#n:_=_ arithmetic expression evaluation#s:= expression#d:Parse and compute an arithmetic expression\n \n.x,+,*,/,%,^: add, subtr, mult, div, modulo, power\n.exp(x): Euler's number 'e' raised to the power of x\n.ln(x),log(x): the natural (resp. base 10) logarithm of x\n.sqrt(x): the correctly rounded positive square root of x\n.ceil(x),floor(x): the smallest (resp. largest) integer value\n.round(x): the value of the argument rounded to the nearest integer\n.abs(x): the absolute value of the argument\n.sin(x),cos(x),tan(x): trigo sin,cosin,tangent of an angle (x in degrees)\n.asin(x),acos(x),atan(x): the arc sin,cosin,tangent(result in radians)\n.sinh(x),cosh(x),tanh(x):the hyperbolic sin,cosin,tangent of x\n.sind,cosd,tand:trigo functions of an angle (x in degress)\n.asind,acosd,atad: the arc trigo functions (result in degrees)\n.toRadians(a): the measurement of the angle a in radians\n.toDegrees(a): the measurement of the angle a in degrees\n.min(x,y),max(x,y): the smaller (resp. larger) of x and y\n.atan2(x,y),atan2d(x,y): the angle (in radians resp. degrees) corresponding to x,y in cartesian coordinates\n.dist(x1,y1,x2,y2): cartesian distance between x1,y1 and x2,y2\n.skydist(ra1,de1,ra2,de2): spherical distance (in degrees or h:m:s +d:m:s)#t:The equal (=) character can be also inserted after the expression#e:= sin(0.5)^2+cos(0.5)^2#e:134*135=
#Help.hipsgen	#n:_hipsgen_ - HEALPix all-sky generation#s:skygen -input=folder ... [cmd]#s:hipsgen abort|pause|resume#d:This command allows one to generate an HEALPix all-sky from a set of images (see menu Tools -> HEALPix all-sky builder for explanation).\n \nBy default all all-sky products are generated, but it is possible to specified explicitely a list of them: index, tiles, jpeg, allsky, moc, tree, gzip, progen.\n The available parameters are: -input:input directory, -output:output directory, -force:clean previous computations, -mode:Coadd mode when restart: pixel level(OVERWRITE|KEEP|AVERAGE) or tile level (REPLACETILE|KEEPTILE) - (default OVERWRITE), -img:Specifical reference image for default initializations (BITPIX,BSCALE,BZERO,BLANK,order,pixelCut,dataCut), -bitpix:Specifical target bitpix, -order: Specifical HEALPix order, -blank:Specifical BLANK value, -skyval:Fits key for removing a sky background, -maxThread: Max number of computing threads, -region: Specifical HEALPix region to compute (ex: 3/34-38 50 53) or Moc.fits file (all sky by default), -jpegMethod: Jpeg HEALPix method (MEDIAN|MEAN) (default MEDIAN), -pixelCut Specifical pixel cut and/or transfert function for JPEG 8 bits conversion - ex: "120 140 log"), -pixelRange: Specifical pixel value range (required for bitpix conversion - ex: "-32000 +32000"), -color: True if the source images are colored jpeg.#e:hipsgen -input=myDir -bitpix=16
Help.test	#n:_test_ - developement tests #s:testimg width height raj dej pxsize proj bitpix#s:testcat width height raj dej pxsize#s:test width height raj dej pxsize proj bitpix#s:testscript#s:testlang#s:testperf [path]#s:testnet [gzip|nogzip] [all] #d:1) Generate an image or/and a table for testing formats, calibration...\n   .width height: image size in pixels\n   .raj dej: coordinates of central pixel\n   .pxsize: pixel size in arcsec\n   .proj SIN, TAN, ARC, AIT, ZEA, STG, CAR, NCP, ZPN\n   .bitpix: pixel FITS coding (8,16,32,-32,-64)\nNote: Two files are generated Test.fits and Text.txt and reloaded in Aladin. The image is a simple pixel grid with a astrometrical calibration corresponding to the parameters . The table contains objects which should be matching the image grid (one object each five pixels in both direction).\n \n2) testscript launchs a script testing all script commands. The result should be\nhttp://aladin.u-strasbg.fr/java/testscript.jpg\n \n3) testlang verify the current translation\n \n4) testperf tests the disk and CPU performances (see stdout for the results)\n \n5) testnet tests the HiPS node network performance (see stdout for the results)#e:test 500 300 0 +0 60 SIN 8#e:testscript#e:testperf /export/home