Path: csiph.com!fu-berlin.de!bofh.it!news.nic.it!robomod From: Ole Streicher 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: X-Mailbox-Line: From debian-bugs-dist-request@lists.debian.org Tue Jul 19 14:15:11 2022 Old-Return-Path: X-Spam-Flag: NO X-Spam-Score: -0.875 Reply-To: Ole Streicher , 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 MIME-Version: 1.0 User-Agent: Mozilla/5.0 (X11; Linux x86_64; rv:91.0) Gecko/20100101 Thunderbird/91.10.0 Content-Language: en-US Organization: Debian Content-Type: text/plain; charset=UTF-8 Content-Transfer-Encoding: 7bit X-Debian-Message: from BTS X-Mailing-List: archive/latest/1725854 List-ID: List-URL: 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 Package: wnpp Severity: wishlist Owner: Ole Streicher 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