Ubuntu
cpl-plugin-visir package

cpl-plugin-visir 4.3.8+dfsg-1 source package in Ubuntu

Changelog

cpl-plugin-visir (4.3.8+dfsg-1) unstable; urgency=low

  * New upstream version 4.3.8+dfsg
  * Push Standards-Version to 4.4.0. No changes required.
  * Push compat to 12. Remove d/compat
  * Add tests on salsa
  * Mark test as superficial
  * Add overrides for visir_img_trans.so and visir_util_convert_weight.so
    not linked to libc

 -- Ole Streicher <email address hidden>  Fri, 23 Aug 2019 14:12:22 +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
Focal release universe misc

Downloads

File Size SHA-256 Checksum
cpl-plugin-visir_4.3.8+dfsg-1.dsc 2.3 KiB 11b86462f4a434e205f321855e487b0edbf71fd858da92b7eb3ea7ba0bd0e032
cpl-plugin-visir_4.3.8+dfsg.orig.tar.xz 2.4 MiB 60e9485c8f0b3f1fac1ef45e9d1cc7501ad157a378575304e30c293a2f361549
cpl-plugin-visir_4.3.8+dfsg-1.debian.tar.xz 11.2 KiB 9712444106c735a8a8b0a9f51f078489dd80ff0090173c560c4b09498b53fda3

No changes file available.

Binary packages built by this source

cpl-plugin-visir: ESO data reduction pipeline for the VISIR instrument

 This is the data reduction pipeline for the Visir instrument of the
 Very Large Telescope (VLT) from the European Southern Observatory (ESO).
 .
 The VLT spectrometer and imager for the mid-infrared (VISIR) was built by
 CEA/DAPNIA/SAP and NFRA/ASTRON, and is located at the Cassegrain focus of
 UT3. It provides diffraction-limited imaging at high sensitivity in the two
 mid infrared (MIR) atmospheric windows: the N band between 8 to 13μm and the Q
 band between 16.5 and 24.5μm, respectively. In addition, it features a
 long-slitspectrometer with a range of spectral resolutions between 150 and
 30000.

cpl-plugin-visir-calib: ESO data reduction pipeline calibration data downloader for VISIR

 This package downloads calibration and other static data of the
 data reduction pipeline for the Visir instrument of the
 Very Large Telescope (VLT) from the European Southern Observatory (ESO).
 .
 The VLT spectrometer and imager for the mid-infrared (VISIR) was built by
 CEA/DAPNIA/SAP and NFRA/ASTRON, and is located at the Cassegrain focus of
 UT3. It provides diffraction-limited imaging at high sensitivity in the two
 mid infrared (MIR) atmospheric windows: the N band between 8 to 13μm and the Q
 band between 16.5 and 24.5μm, respectively. In addition, it features a
 long-slitspectrometer with a range of spectral resolutions between 150 and
 30000.

cpl-plugin-visir-dbgsym: No summary available for cpl-plugin-visir-dbgsym in ubuntu groovy.

No description available for cpl-plugin-visir-dbgsym in ubuntu groovy.

cpl-plugin-visir-doc: No summary available for cpl-plugin-visir-doc in ubuntu groovy.

No description available for cpl-plugin-visir-doc in ubuntu groovy.