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Groups > linux.debian.maint.python > #14256
| Path | csiph.com!fu-berlin.de!bofh.it!news.nic.it!robomod |
|---|---|
| From | Ole Streicher <olebole@debian.org> |
| Newsgroups | linux.debian.bugs.dist, linux.debian.devel, linux.debian.maint.python |
| Subject | Bug#1015324: ITP: synphot -- Simulate photometric data ans spectra in astronomy |
| Date | Tue, 19 Jul 2022 16:20:01 +0200 |
| Message-ID | <EKWeR-cpIY-1@gated-at.bofh.it> (permalink) |
| X-Mailbox-Line | From debian-bugs-dist-request@lists.debian.org Tue Jul 19 14:15:11 2022 |
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| Reply-To | Ole Streicher <olebole@debian.org>, 1015324@bugs.debian.org |
| Resent-To | debian-bugs-dist@lists.debian.org |
| Resent-Cc | debian-devel@lists.debian.org, debian-astro@lists.debian.org, debian-python@lists.debian.org, wnpp@debian.org |
| X-Debian-Pr-Message | report 1015324 |
| X-Debian-Pr-Package | wnpp |
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| Organization | Debian |
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| X-Mailing-List | <debian-bugs-dist@lists.debian.org> archive/latest/1725854 |
| List-ID | <debian-bugs-dist.lists.debian.org> |
| List-URL | <https://lists.debian.org/debian-bugs-dist/> |
| Approved | robomod@news.nic.it |
| Lines | 39 |
| Sender | robomod@news.nic.it |
| X-Original-Date | Tue, 19 Jul 2022 16:12:03 +0200 |
| X-Original-Message-ID | <2764949c-05da-8554-d2ec-52d16d8903aa@debian.org> |
| Xref | csiph.com linux.debian.bugs.dist:1110338 linux.debian.devel:105064 linux.debian.maint.python:14256 |
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Package: wnpp Severity: wishlist Owner: Ole Streicher <olebole@debian.org> X-Debbugs-Cc: debian-devel@lists.debian.org, debian-astro@lists.debian.org, debian-python@lists.debian.org Control: block 1012441 by -1 * Package name : synphot Version : 1.1.2 Upstream Author : Space Telescope Science Institute * URL : https://github.com/spacetelescope/synphot_refactor * License : BSD-3-Clause Programming Lang: Python 3 Description : Simulate photometric data ans 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. This is a dependency of the upcoming specreduce package (ITP #1012441). I will maintain the package within the Debian Astro team in Salsa: https://salsa.debian.org/debian-astro-team/synphot Best regards Ole
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Bug#1015324: ITP: synphot -- Simulate photometric data ans spectra in astronomy Ole Streicher <olebole@debian.org> - 2022-07-19 16:20 +0200
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