1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261
|
.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.49.3.
.TH SEGMENT "1" "November 2025" "GNU Astronomy Utilities 0.24" "User Commands"
.SH NAME
Segment \- segmentation based on signal structure
.SH SYNOPSIS
.B astsegment
[\fI\,OPTION\/\fR...] \fI\,ASTRdata\/\fR
.SH DESCRIPTION
Segment is part of GNU Astronomy Utilities 0.24.
Segment will segment an initially labeled region based on structure with the
signal. It will first find true clumps (local maxima), estimate which ones have
strong connections, and then grow them to cover the full area of each
detection.
.PP
For more information, please run any of the following commands. In particular
the second contains a very comprehensive explanation of Segment's invocation:
expected input(s), output(s), and a full description of all the options.
.TP
All options and their values:
$ astsegment \fB\-P\fR
.TP
Inputs/Outputs and options:
$ info astsegment
.TP
Full section in manual/book:
$ info Segment
.TP
Full Gnuastro manual/book:
$ info gnuastro
.PP
If you couldn't find your answer in the manual, you can get direct help from
experienced Gnuastro users and developers. For more information, please run:
.IP
\f(CW$ info help-gnuastro\fR
.PP
Segment options:
.IP
Input:
.TP
\fB\-\-chdu\fR=\fI\,STR\/\fR
HDU/extension of convolved image in file.
.TP
\fB\-\-convolved\fR=\fI\,FITS\/\fR
Convolved image file to avoid convolution.
.TP
\fB\-\-dhdu\fR=\fI\,STR\/\fR
HDU containing detection image.
.TP
\fB\-d\fR, \fB\-\-detection\fR=\fI\,FITS\/\fR
Filename of detection image (to segment).
.TP
\fB\-h\fR, \fB\-\-hdu\fR=\fI\,STR\/\fR/INT
HDU containing values (science image).
.TP
\fB\-\-khdu\fR=\fI\,STR\/\fR
HDU containing kernel image.
.TP
\fB\-k\fR, \fB\-\-kernel\fR=\fI\,FITS\/\fR
Filename of kernel to convolve with input.
.TP
\fB\-\-sky\fR=\fI\,STR\/\fR/FLT
Filename of Sky values image to subtract.
.TP
\fB\-\-skyhdu\fR=\fI\,STR\/\fR
HDU containing Sky value to subtract.
.TP
\fB\-\-std\fR=\fI\,STR\/\fR/FLT
Filename of Sky standard deviation.
.TP
\fB\-\-stdhdu\fR=\fI\,STR\/\fR
HDU containing Sky standard deviation.
.TP
\fB\-\-variance\fR
STD input is actually variance.
.IP
Tessellation (tile grid):
.TP
\fB\-\-checktiles\fR
Tile IDs in an image, the size of input.
.TP
\fB\-F\fR, \fB\-\-remainderfrac\fR=\fI\,FLT\/\fR
Fraction of remainder to split last tile.
.TP
\fB\-\-interpmetric\fR=\fI\,STR\/\fR
Interpolation metric (radial, manhattan).
.TP
\fB\-\-interpnumngb\fR=\fI\,INT\/\fR
No. of neighbors to use for interpolation.
.TP
\fB\-\-interponlyblank\fR
Only interpolate over the blank tiles.
.TP
\fB\-L\fR, \fB\-\-largetilesize\fR=\fI\,INT[\/\fR,INT]
Sim. to \fB\-\-tilesize\fR, but for larger tiles.
.HP
\fB\-M\fR, \fB\-\-numchannels\fR=\fI\,INT[\/\fR,..] No. of channels in dim.s (FITS order).
.TP
\fB\-\-oneelempertile\fR
Display 1 element/tile, not full input res.
.TP
\fB\-\-workoverch\fR
Work (not tile) over channel edges.
.TP
\fB\-Z\fR, \fB\-\-tilesize\fR=\fI\,INT[\/\fR,INT]
Regular tile size on dim.s (FITS order).
.IP
Output:
.TP
\fB\-D\fR, \fB\-\-dontdelete\fR
Don't delete output if it exists.
.TP
\fB\-K\fR, \fB\-\-keepinputdir\fR
Keep input directory for automatic output.
.TP
\fB\-\-noobjects\fR
Finish with true clumps, don't create objects.
.TP
\fB\-\-outfitsnocommit\fR
No Git commit in 0\-th HDU of output FITS.
.TP
\fB\-\-outfitsnoconfig\fR
No metadata in 0\-th HDU of output FITS.
.TP
\fB\-\-outfitsnodate\fR
No 'DATE' in 0\-th HDU of output FITS.
.TP
\fB\-\-outfitsnoversions\fR
No versions in 0\-th HDU of output FITS.
.TP
\fB\-o\fR, \fB\-\-output\fR=\fI\,STR\/\fR
Output file name.
.TP
\fB\-\-rawoutput\fR
Output contains only CLUMPS and/or OBJECTS HDUs.
.TP
\fB\-\-tableformat\fR=\fI\,STR\/\fR
\&'txt', 'fits\-ascii', 'fits\-binary'.
.TP
\fB\-\-wcslinearmatrix\fR=\fI\,STR\/\fR
WCS linear matrix of output ('pc' or 'cd').
.IP
Segmentation:
.TP
\fB\-B\fR, \fB\-\-minskyfrac\fR=\fI\,FLT\/\fR
Min. fraction of undetected area in tile.
.TP
\fB\-\-checksegmentation\fR
Store segmentation steps in a file.
.TP
\fB\-\-checksn\fR
Save clump S/N values into a file.
.TP
\fB\-c\fR, \fB\-\-snquant\fR=\fI\,FLT\/\fR
S/N Quantile of true sky clumps.
.TP
\fB\-\-grownclumps\fR
Save grown clumps instead of original.
.TP
\fB\-G\fR, \fB\-\-gthresh\fR=\fI\,FLT\/\fR
Multiple of STD to stop growing clumps.
.TP
\fB\-\-minima\fR
Built internal clumps from minima.
.TP
\fB\-\-minnumfalse\fR=\fI\,INT\/\fR
Minimum number for S/N estimation.
.TP
\fB\-m\fR, \fB\-\-snminarea\fR=\fI\,INT\/\fR
Minimum area of clumps for S/N estimation.
.TP
\fB\-O\fR, \fB\-\-objbordersn\fR=\fI\,FLT\/\fR
Min. S/N for grown clumps as one object.
.TP
\fB\-s\fR, \fB\-\-clumpsnthresh\fR=\fI\,FLT\/\fR
S/N threshold of true clumps.
.TP
\fB\-v\fR, \fB\-\-keepmaxnearriver\fR
Keep clumps with peak touching a river.
.TP
\fB\-y\fR, \fB\-\-minriverlength\fR=\fI\,INT\/\fR
Minimum len of useful grown clump rivers.
.IP
Operating modes:
.TP
\-?, \fB\-\-help\fR
give this help list
.TP
\fB\-\-checkconfig\fR
List all config files and variables read.
.TP
\fB\-\-cite\fR
BibTeX citation for this program.
.TP
\fB\-\-config\fR=\fI\,STR\/\fR
Read configuration file STR immediately.
.TP
\fB\-\-config\-prefix\fR=\fI\,STR\/\fR
Custom prefix of option names config files.
.TP
\fB\-C\fR, \fB\-\-continueaftercheck\fR
Continue processing after checks.
.TP
\fB\-\-lastconfig\fR
Do not parse any more configuration files.
.TP
\fB\-\-minmapsize\fR=\fI\,INT\/\fR
Min. bytes to avoid RAM automatically.
.TP
\fB\-N\fR, \fB\-\-numthreads\fR=\fI\,INT\/\fR
Number of CPU threads to use.
.TP
\fB\-\-onlyversion\fR=\fI\,STR\/\fR
Only run if the program version is STR.
.TP
\fB\-P\fR, \fB\-\-printparams\fR
Print parameter values to be used and abort.
.TP
\fB\-\-quietmmap\fR
Don't print mmap'd file's name and size.
.TP
\fB\-q\fR, \fB\-\-quiet\fR
Only report errors, remain quiet about steps.
.TP
\fB\-S\fR, \fB\-\-setdirconf\fR
Set default values for this directory and abort.
.TP
\fB\-\-usage\fR
give a short usage message
.TP
\fB\-U\fR, \fB\-\-setusrconf\fR
Set default values for this user and abort.
.TP
\fB\-V\fR, \fB\-\-version\fR
print program version
.PP
Mandatory or optional arguments to long options are also mandatory or optional
for any corresponding short options.
.PP
GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/
.SH "REPORTING BUGS"
Report bugs to bug\-gnuastro@gnu.org.
.SH COPYRIGHT
Copyright \(co 2015\-2025 Free Software Foundation, Inc.
License GPLv3+: GNU General public license version 3 or later.
.br
This is free software: you are free to change and redistribute it.
There is NO WARRANTY, to the extent permitted by law.
.PP
Written/developed by Mohammad Akhlaghi
.SH "SEE ALSO"
The full documentation for
.B Segment
is maintained as a Texinfo manual. If the
.B info
and
.B Segment
programs are properly installed at your site, the command
.IP
.B info Segment
.PP
should give you access to the complete manual.
|