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[ Source: synphot  ]

Package: python3-synphot (1.1.1-3 and others)

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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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Download for all available architectures
Architecture Version Package Size Installed Size Files
amd64 1.1.1-3+b2 603.1 kB1,623.0 kB [list of files]
arm64 1.1.1-3+b2 590.7 kB1,675.0 kB [list of files]
armel 1.1.1-3+b2 591.3 kB1,622.0 kB [list of files]
armhf 1.1.1-3+b2 590.6 kB1,618.0 kB [list of files]
i386 1.1.1-3+b2 600.4 kB1,622.0 kB [list of files]
mips64el 1.1.1-3+b2 589.7 kB1,675.0 kB [list of files]
mipsel 1.1.1-3+b2 595.3 kB1,674.0 kB [list of files]
ppc64el 1.1.1-3+b2 589.8 kB1,675.0 kB [list of files]
s390x 1.1.1-3+b2 600.7 kB1,619.0 kB [list of files]