cpl-plugin-muse 1.0.4+dfsg-4 source package in Ubuntu

Changelog

cpl-plugin-muse (1.0.4+dfsg-4) unstable; urgency=low

  * Reproducibly sort recipes in sphinx output. Closes: #792938

 -- Ole Streicher <email address hidden>  Mon, 20 Jul 2015 15:09:10 +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_1.0.4+dfsg-4.dsc 2.3 KiB 8f2ee5dd04e05098d815a8212dc21265e53ecf1a1d888d9001e8f4f508e45719
cpl-plugin-muse_1.0.4+dfsg.orig.tar.xz 914.7 KiB d86d78a3510f273d5dd44b91b19a1eccf0d02d759bb6fa61367fb2189ed64537
cpl-plugin-muse_1.0.4+dfsg-4.debian.tar.xz 12.0 KiB 6a99db749f462da48e011d70ff6e9d119cbc9d3cd69a3ad59d1f2fcae73c11b8

Available diffs

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-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 package cpl-plugin-muse

 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-doc: No summary available for cpl-plugin-muse-doc in ubuntu wily.

No description available for cpl-plugin-muse-doc in ubuntu wily.