cpl-plugin-muse 1.2.1+dfsg-2 source package in Ubuntu

Changelog

cpl-plugin-muse (1.2.1+dfsg-2) unstable; urgency=low

  * Fix FTBS on i386

 -- Ole Streicher <email address hidden>  Tue, 13 Oct 2015 22:00:41 +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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Series Pocket Published Component Section
Xenial release universe misc

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File Size SHA-256 Checksum
cpl-plugin-muse_1.2.1+dfsg-2.dsc 2.3 KiB 74b10e9bae8ad9720960216f9a56ac79ca7c01b7a3cd00ca475dbf819a659e54
cpl-plugin-muse_1.2.1+dfsg.orig.tar.xz 1005.9 KiB 9ad69e519ff6daee1a842f79ce6821b6c7a5b0adcd6663b86df99c529714549f
cpl-plugin-muse_1.2.1+dfsg-2.debian.tar.xz 11.7 KiB 98fcb8177a9187ca676ce0a42f2db7ca459fcdd1e2444c6e44ccc00bfc976e43

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: 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).