Ubuntu
synphot package

synphot 1.2.1-1 source package in Ubuntu

Changelog

synphot (1.2.1-1) unstable; urgency=medium

  * Add ASCL-Id to d/u/metadata
  * Correct homepage URL
  * New upstream version 1.2.1
  * Drop Enforce-little-endian-when-reading-Numpy-test-data-file.patch:
    applied upstream
  * Push Standards-Version to 4.6.2. No changes needed

 -- Ole Streicher <email address hidden>  Sat, 24 Jun 2023 12:22:54 +0200

Upload details

Uploaded by:
Debian Astronomy Maintainers
Uploaded to:
Sid
Original maintainer:
Debian Astronomy Maintainers
Architectures:
any
Section:
misc
Urgency:
Medium Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Mantic release universe misc

Downloads

File Size SHA-256 Checksum
synphot_1.2.1-1.dsc 2.1 KiB c2140f737d79cf8d629b6ff2f355c933c4f6eae0525e92087b1b1ba9329f5ddf
synphot_1.2.1.orig.tar.gz 1.3 MiB 84b1b35024f0db11b487c86810289dc3b9c57f743075a9a1e02156fcc46b6c82
synphot_1.2.1-1.debian.tar.xz 3.2 KiB 8f154f2f81cd20f51970922ee0f85dff2817e80562fef51b303898927bce5b95

No changes file available.

Binary packages built by this source

python3-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.

python3-synphot-dbgsym: debug symbols for python3-synphot