synphot 1.2.1-1build1 source package in Ubuntu
Changelog
synphot (1.2.1-1build1) noble; urgency=medium * No-change rebuild with Python 3.12 as supported version -- Graham Inggs <email address hidden> Fri, 03 Nov 2023 11:32:27 +0000
Upload details
- Uploaded by:
- Graham Inggs
- Uploaded to:
- Noble
- Original maintainer:
- Debian Astronomy Maintainers
- Architectures:
- any
- Section:
- misc
- Urgency:
- Medium Urgency
See full publishing history Publishing
Series | Published | Component | Section | |
---|---|---|---|---|
Noble | release | universe | misc |
Downloads
File | Size | SHA-256 Checksum |
---|---|---|
synphot_1.2.1.orig.tar.gz | 1.3 MiB | 84b1b35024f0db11b487c86810289dc3b9c57f743075a9a1e02156fcc46b6c82 |
synphot_1.2.1-1build1.debian.tar.xz | 3.2 KiB | db8e66c7bd29ce4b967730bc1fef813f82682d144adf213f2913c23be65a4869 |
synphot_1.2.1-1build1.dsc | 2.2 KiB | 3063f953c7182bf14992cd91c15f79180d853891ea893bff6a2e9e1962348689 |
Available diffs
- diff from 1.2.1-1 (in Debian) to 1.2.1-1build1 (323 bytes)
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