cpl-plugin-fors 5.3.32+dfsg-1 source package in Ubuntu

Changelog

cpl-plugin-fors (5.3.32+dfsg-1) unstable; urgency=low

  * Update VCS fields to use salsa.d.o
  * Use name-based sorting for the recipes to ensure reproducible build
  * New upstream version 5.3.32+dfsg. Rediff patches
  * Push Standards-Version to 4.1.4. Change remaining URLs to https
  * Push compat to 11
  * Switch to Python 3
  * Adjust documentation path

 -- Ole Streicher <email address hidden>  Wed, 25 Apr 2018 15:44:46 +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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cpl-plugin-fors_5.3.32+dfsg-1.dsc 2.3 KiB bb2e5e6d8db48ad033194455773e9b3e85939aca817b61ab7e92e670e86953fb
cpl-plugin-fors_5.3.32+dfsg.orig.tar.xz 1.0 MiB 68e1db2482d4ff73487232113a1112a839edb1f9d4cc3e4997e2d2cb06c90b84
cpl-plugin-fors_5.3.32+dfsg-1.debian.tar.xz 11.4 KiB 2420951ac2f39dfbdeb13eb52b574db2a2bd5cf5d6e1b9834e8f5e761dc464aa

No changes file available.

Binary packages built by this source

cpl-plugin-fors: ESO data reduction pipeline for the FORS1/2 instruments

 FORS pipeline recipes for the reduction of data obtained with the FORS1 and
 FORS2 instruments in the LSS, MOS, MXU, PMOS, and direct imaging instrument
 modes.
 .
 FORS is the visual and near UV FOcal Reducer and low dispersion Spectrograph
 for the Very Large Telescope (VLT) of the European Southern Observatory
 (ESO). Two versions of FORS have been built, upgraded and moved to the
 Cassegrain foci of different telescopes in the past years. In April 2009,
 FORS1 was dismounted to make room for X-shooter, so only FORS2 is in
 operation. FORS is designed as an all-dioptric instrument for the wavelength
 range from 330 nm to 1100 nm and provides an image scale of 0".25/pixel (or
 0".125/pixel with the high resolution collimator) in the standard readout
 mode (2x2 binning). FORS2 is installed on UT1 (Antu) and is by default
 equipped with a detector system that is optimised for the red with a very low
 level of fringes thanks to a mosaic of two 2k x 4k MIT CCDs (with 15 μm
 pixels). However, the blue-optimised detector system that was previously
 available on FORS1 has been commissioned on FORS2 and can be requested for
 Visitor Mode observation. The geometries of both detector systems are
 similar, with the optical axis falling ~30" above the gap and offsets of a
 few arc-seconds between the two chips. FORS2 has many modes, including
 multi-object spectroscopy with exchangeable masks, long-slit spectroscopy,
 imaging and spectro-polarimetry and high-time resolution imaging and
 spectroscopy.

cpl-plugin-fors-calib: No summary available for cpl-plugin-fors-calib in ubuntu eoan.

No description available for cpl-plugin-fors-calib in ubuntu eoan.

cpl-plugin-fors-dbgsym: debug symbols for cpl-plugin-fors
cpl-plugin-fors-doc: ESO data reduction pipeline documentation for FORS

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