synphot 1.3.0-1build1 source package in Ubuntu
Changelog
synphot (1.3.0-1build1) noble; urgency=medium * No-change rebuild with Python 3.12 only -- Graham Inggs <email address hidden> Wed, 10 Apr 2024 15:31:35 +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_1.3.0.orig.tar.gz | 1.3 MiB | 5bf3f8e415ac83d44c0727fb7257db33b09262af850c0cf1100f2a70a319a814 |
| synphot_1.3.0-1build1.debian.tar.xz | 3.2 KiB | a72ca60c5b34fdb831b94512c8d1da2677bb87411573051f3c9f5c4eadcc2486 |
| synphot_1.3.0-1build1.dsc | 2.2 KiB | d65c23175b9d23b9cb9f36243e5139d493eaf43b3256bb83fa4f2e1c660aef07 |
Available diffs
- diff from 1.3.0-1 (in Debian) to 1.3.0-1build1 (309 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
