cpl-plugin-muse 2.8+dfsg-1 source package in Ubuntu

Changelog

cpl-plugin-muse (2.8+dfsg-1) unstable; urgency=low

  * New upstream version 2.8+dfsg. Rediff patches
  * Mark CI test as superficial

 -- Ole Streicher <email address hidden>  Tue, 08 Oct 2019 13:23:54 +0200

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

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File Size SHA-256 Checksum
cpl-plugin-muse_2.8+dfsg-1.dsc 2.3 KiB 8b947f31b09685d6a02bb64476a1fab88cea5e40082df606a2e1d0905f650a2e
cpl-plugin-muse_2.8+dfsg.orig.tar.xz 1.1 MiB 19aedf05665962d00582a37f0d6ba92a6e63f7b9f17000c716b4da9e46676a11
cpl-plugin-muse_2.8+dfsg-1.debian.tar.xz 13.2 KiB bac835eecfe2347e9dcab65618f5ca966d5048d69ed7b01a94e4316a53e2effb

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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-calib: ESO data reduction pipeline calibration data downloader for MUSE

 This package downloads calibration and other static data of 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
cpl-plugin-muse-doc: ESO data reduction pipeline documentation for MUSE

 This package contains the HTML documentation and manpages for the data
 reduction pipeline for the Muse instrument of the Very Large Telescope
 (VLT) from the European Southern Observatory (ESO).