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cpl-plugin-vimos package

cpl-plugin-vimos 2.9.15+dfsg-4 source package in Ubuntu

Changelog

cpl-plugin-vimos (2.9.15+dfsg-4) unstable; urgency=low

  * Limit CI test dependency to plugin

 -- Ole Streicher <email address hidden>  Wed, 20 May 2015 09:28:20 +0200

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-vimos_2.9.15+dfsg-4.dsc 2.3 KiB 1ea7b1838b268056d376d017620556802ea39bdc1138baad4e739aa927ab9bfb
cpl-plugin-vimos_2.9.15+dfsg.orig.tar.xz 1.3 MiB dfdf1f868affa21e06b2ef296fa8b2a0aa31ab6dd168835996b83dba5a65d652
cpl-plugin-vimos_2.9.15+dfsg-4.debian.tar.xz 13.6 KiB d0d3f376fa82a543e174749dc3189245223137d2ce5a435966f70d2658f93747

No changes file available.

Binary packages built by this source

cpl-plugin-vimos: ESO data reduction pipeline for VIMOS

 This is the data reduction pipeline for the Vimos instrument of the
 Very Large Telescope (VLT) from the European Southern Observatory (ESO).
 .
 VIMOS is a multi-mode wide-field optical instrument mounted at the Nasmyth
 focus B of UT3. VIMOS allows imaging in UBVRIz and multi-object low (R ~ 200)
 to high (R ~ 2500) resolution spectroscopy. The wavelength range covered in
 the two spectroscopic modes goes from 360 to 1000 nm. VIMOS is made of 4
 quadrants of 7'x8' each separated by a gap of about 2'.

cpl-plugin-vimos-calib: No summary available for cpl-plugin-vimos-calib in ubuntu wily.

No description available for cpl-plugin-vimos-calib in ubuntu wily.

cpl-plugin-vimos-dbgsym: debug symbols for package cpl-plugin-vimos

 This is the data reduction pipeline for the Vimos instrument of the
 Very Large Telescope (VLT) from the European Southern Observatory (ESO).
 .
 VIMOS is a multi-mode wide-field optical instrument mounted at the Nasmyth
 focus B of UT3. VIMOS allows imaging in UBVRIz and multi-object low (R ~ 200)
 to high (R ~ 2500) resolution spectroscopy. The wavelength range covered in
 the two spectroscopic modes goes from 360 to 1000 nm. VIMOS is made of 4
 quadrants of 7'x8' each separated by a gap of about 2'.

cpl-plugin-vimos-doc: ESO data reduction pipeline documentation for VIMOS

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