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Package: python3-synphot (1.4.0-1)

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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 Package Size Installed Size Files
alpha (unofficial port) 597.2 kB1,768.0 kB [list of files]
amd64 597.3 kB1,664.0 kB [list of files]
arm64 595.7 kB1,768.0 kB [list of files]
armel 608.8 kB1,662.0 kB [list of files]
armhf 596.3 kB1,654.0 kB [list of files]
hppa (unofficial port) 595.7 kB1,656.0 kB [list of files]
i386 599.7 kB1,662.0 kB [list of files]
m68k (unofficial port) 609.4 kB1,654.0 kB [list of files]
mips64el 597.2 kB1,768.0 kB [list of files]
ppc64 (unofficial port) 603.5 kB1,768.0 kB [list of files]
ppc64el 606.0 kB1,768.0 kB [list of files]
riscv64 606.9 kB1,656.0 kB [list of files]
s390x 599.2 kB1,656.0 kB [list of files]
sh4 (unofficial port) 595.9 kB1,766.0 kB [list of files]