Paketti: python3-synphot (1.4.0-1) [debports]

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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.

Muut pakettiin python3-synphot liittyvät paketit

• dep: libc6 (>= 2.2)

  GNU-C-kirjasto: jaetut kirjastot
  myös näennäispaketti, jonka toteuttaa libc6-udeb

• dep: python3

  interactive high-level object-oriented language (default python3 version)

  dep: python3 (<< 3.13)

  dep: python3 (>= 3.11~)

• dep: python3-astropy

  Core functionality for performing astrophysics with Python

• dep: python3-numpy (>= 1:1.25.0)

  Fast array facility to the Python language (Python 3)

• dep: python3-numpy-abi9

  näennäispaketti, jonka toteuttaa python3-numpy

• dep: python3-scipy

  scientific tools for Python 3

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