[ 原始碼： synphot ]
套件：python3-synphot（1.1.1-3 以及其他的）
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
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- 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
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- dep: python3
- interactive high-level object-oriented language (default python3 version)
- dep: python3 (<< 3.12)
- dep: python3 (>= 3.11~)
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- dep: python3-astropy
- Core functionality for performing astrophysics with Python
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- dep: python3-numpy (>= 1:1.22.0)
- Fast array facility to the Python 3 language
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- dep: python3-numpy-abi9
- 本虛擬套件由這些套件填實： python3-numpy
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- dep: python3-scipy
- scientific tools for Python 3