套件：python3-synphot（1.4.0-1 以及其他的）

[ 原始碼： synphot  ]

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.

其他與 python3-synphot 有關的套件

• dep: libc6 (>= 2.4)

  GNU C 函式庫：共用函式庫
  同時作為一個虛擬套件由這些套件填實： libc6-udeb

• dep: python3

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

  dep: python3 (<< 3.13)

  dep: python3 (>= 3.12~)

• 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

  本虛擬套件由這些套件填實： python3-numpy

• dep: python3-scipy

  scientific tools for Python 3

下載 python3-synphot

下載可用於所有硬體架構的

硬體架構	版本	套件大小	安裝後大小	檔案
armel	1.4.0-1+b1	597。4 kB	1，649。0 kB	[檔案列表]