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Source: synphot
Standards-Version: 4.7.3
Maintainer: Debian Astronomy Team <debian-astro-maintainers@lists.alioth.debian.org>
Uploaders:
Ole Streicher <olebole@debian.org>,
Section: python
Priority: optional
Build-Depends:
debhelper-compat (= 13),
dh-python,
python3-all-dev,
python3-astropy,
python3-numpy,
python3-numpy-dev,
python3-pytest,
python3-pytest-astropy,
python3-scipy,
python3-setuptools,
python3-setuptools-scm,
Vcs-Browser: https://salsa.debian.org/debian-astro-team/synphot
Vcs-Git: https://salsa.debian.org/debian-astro-team/synphot.git
Homepage: https://github.com/spacetelescope/synphot_refactor
Package: python3-synphot
Architecture: any
Depends:
${misc:Depends},
${python3:Depends},
${shlibs:Depends},
Description: Simulate photometric data and spectra in astronomy
Synphot simulates photometric data and spectra, observed or otherwise.
It can incorporate external filters, spectra, and data. One can also use
a pre-defined standard star (Vega), bandpass, or extinction law.
Furthermore, it allows one to:
.
* Construct complicated composite spectra using different models.
* Simulate observations.
* Compute photometric properties such as count rate, effective
wavelength, and effective stimulus.
* Manipulate a spectrum; e.g., applying redshift or normalize it to a
given flux value in a given bandpass.
* Sample a spectrum at given wavelengths.
* Plot a quick-view of a spectrum.
* Perform repetitive operations such as simulating the observations of
multiple type of sources through multiple bandpasses.
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