套件:python3-pysynphot(2.0.0+dfsg-1 以及其他的)
python3-pysynphot 的相關連結
Debian 的資源:
下載原始碼套件 pysynphot:
- [pysynphot_2.0.0+dfsg-1.dsc]
- [pysynphot_2.0.0+dfsg.orig.tar.xz]
- [pysynphot_2.0.0+dfsg-1.debian.tar.xz]
維護小組:
外部的資源:
- 主頁 [ssb.stsci.edu]
相似套件:
Python Synthetic Photometry Utilities
pysynphot simulates photometric data and spectra as they are observed with the Hubble Space Telescope (HST). Passbands for standard photometric systems are available, and users can incorporate their own filters, spectra, and data. pysynphot user interface allows you to:
* Construct complicated composite spectra from various grids of model atmosphere spectra, parameterized spectrum models, and atlases of stellar spectrophotometry. * Simulate observations. * Query the resulting structures for quantities of interest, such as countrate, effective wavelength, effective stimulus, as well as the wavelength and flux arrays. * Plot HST sensitivity curves and calibration target spectra. * Compute photometric calibration parameters for any HST instrument mode.
pysynphot can help HST observers to perform cross-instrument simulations, to examine the transmission curve of the HST Optical Telescope Assembly (OTA), and spectra of HST calibration targets. Expert users can take advantage of the control and data structures available in Python to easily perform repetitive operations such as simulate the observation of multiple type of sources through multiple observing modes.
其他與 python3-pysynphot 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 (<< 3.14)
- dep: python3 (>= 3.12~)
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- dep: python3-astropy
- Core functionality for performing astrophysics with Python
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- dep: python3-bs4
- error-tolerant HTML parser for Python 3
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- dep: python3-numpy (>= 1:1.25.0)
- Fast array facility to the Python language (Python 3)
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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-six
- Python 2 and 3 compatibility library