cpl-plugin-hawki 2.4.6+dfsg-1build1 source package in Ubuntu

Changelog

cpl-plugin-hawki (2.4.6+dfsg-1build1) focal; urgency=medium

  * No-change rebuild for libgcc-s1 package name change.

 -- Matthias Klose <email address hidden>  Sun, 22 Mar 2020 16:36:57 +0100

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Uploaded by:
Matthias Klose
Uploaded to:
Focal
Original maintainer:
Debian Astronomy Maintainers
Architectures:
any all
Section:
misc
Urgency:
Medium Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Focal release universe misc

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File Size SHA-256 Checksum
cpl-plugin-hawki_2.4.6+dfsg.orig.tar.xz 864.1 KiB 541a31f07f2fe08135dbc123319c3769534f0f50a9a3cf1b07df5908789d7526
cpl-plugin-hawki_2.4.6+dfsg-1build1.debian.tar.xz 9.6 KiB ab16bdc520ddca4ea437df496d8dc22294b851928f5bf65f775e722b19546c65
cpl-plugin-hawki_2.4.6+dfsg-1build1.dsc 2.4 KiB a73f45c9b57b5b3e9e687faec96637f722a8441ed80cbcbafab91a0ea6f25ce6

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Binary packages built by this source

cpl-plugin-hawki: ESO data reduction pipeline for the HAWK-I instrument

 This is the data reduction pipeline for the HAWK-I instrument of the
 Very Large Telescope (VLT) from the European Southern Observatory (ESO).
 .
 HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being
 offered for the first time in Period 81. The instrument is cryogenic (120 K,
 detectors at 80 K) and has a full reflective design. The light passes four
 mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048
 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky
 corresponds to 169 μm on the detector).

cpl-plugin-hawki-calib: No summary available for cpl-plugin-hawki-calib in ubuntu groovy.

No description available for cpl-plugin-hawki-calib in ubuntu groovy.

cpl-plugin-hawki-dbgsym: debug symbols for cpl-plugin-hawki
cpl-plugin-hawki-doc: No summary available for cpl-plugin-hawki-doc in ubuntu groovy.

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