cpl-plugin-hawki binary package in Ubuntu Xenial arm64
This is the data reduction pipeline for the HAWK-I instrument of the
Very Large Telescope (VLT) from the European Southern Observatory (ESO).
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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).
Publishing history
Date | Status | Target | Component | Section | Priority | Phased updates | Version | ||
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2015-12-08 18:15:20 UTC | Published | Ubuntu Xenial arm64 | release | universe | science | Optional | 1.8.18+dfsg-5 | ||
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Deleted | Ubuntu Xenial arm64 | proposed | universe | science | Optional | 1.8.18+dfsg-5 | |||
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2015-12-08 18:24:41 UTC | Superseded | Ubuntu Xenial arm64 | release | universe | science | Optional | 1.8.18+dfsg-4build1 | ||
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2015-12-10 00:10:12 UTC | Deleted | Ubuntu Xenial arm64 | proposed | universe | science | Optional | 1.8.18+dfsg-4build1 | ||
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2015-11-13 12:20:14 UTC | Superseded | Ubuntu Xenial arm64 | release | universe | science | Optional | 1.8.18+dfsg-4 | ||
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