Ubuntu
cpl-plugin-muse package

cpl-plugin-muse 2.2+dfsg-1 source package in Ubuntu

Changelog

cpl-plugin-muse (2.2+dfsg-1) unstable; urgency=low

  * New upstream version 2.2+dfsg
  * Push Standards-Version to 4.1.1. Use https in d/watch and d/control
  * Switch to Python 3 in build

 -- Ole Streicher <email address hidden>  Sat, 28 Oct 2017 14:38:58 -0300

Upload details

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

See full publishing history Publishing

Series Pocket Published Component Section

Downloads

File Size SHA-256 Checksum
cpl-plugin-muse_2.2+dfsg-1.dsc 2.3 KiB e78b20456246f13949bb3f13d9cddd67bacf96291b8613a42364cc9be1cfcd34
cpl-plugin-muse_2.2+dfsg.orig.tar.xz 1.1 MiB a14726fea9362db90f0880a58a7ec37bfd02d106ebf24fd3caf23128125fd6ca
cpl-plugin-muse_2.2+dfsg-1.debian.tar.xz 12.8 KiB fee1d61ce39200cd2ac224b3ec40fec4369b1d291706619e5d3a8afcb7c83fc8

No changes file available.

Binary packages built by this source

cpl-plugin-muse: ESO data reduction pipeline for the MUSE instrument

 This is the data reduction pipeline for the Muse instrument of the
 Very Large Telescope (VLT) from the European Southern Observatory (ESO).
 .
 MUSE, the Multi-Unit Spectroscopic Explorer, is an Integral Field
 Spectrograph located at the Nasmyth B focus of Yepun, the VLT UT4
 telescope. It has a modular structure composed of 24 identical IFU modules
 that together sample, in Wide Field Mode (WFM), a near-contiguous 1 squared
 arcmin field of view. Spectrally the instrument samples almost the full
 optical domain with a mean resolution of 3000. Spatially, the instrument
 samples the sky with 0.2 arcseconds spatial pixels in the currently offered
 Wide Field Mode with natural seeing (WFM-noAO).

cpl-plugin-muse-dbgsym: debug symbols for cpl-plugin-muse