Result for 0C4ABCD18EA2B2AF820A137A685F3EA3BD8D941F

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_cal_distortion.so
FileSize26956
MD5F00A3890F94F97E5BFF20A08067CC334
SHA-10C4ABCD18EA2B2AF820A137A685F3EA3BD8D941F
SHA-256D33B583D667A93E1F59AAF0ACF84ECC3219476E6A9C19BA404C9F24AD5FA2441
SSDEEP384:mNb8pClOfD2ggTjNltlCH8TcJkrNHQ49SR9Pwy91bwhm0K4qvZDNF0Se5hsc:5pCl2D2fTRlHCc0kJw49SR90hmcgj
TLSHT143C2F9DEC581EA72D9E312B66C57212965F54500D737C3C2AE0F39892A2265CFE3263F
hashlookup:parent-total1
hashlookup:trust55

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Parents (Total: 1)

The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize255070
MD560BA19F6BF0377B8FBA3875CEE3462A5
PackageDescriptionESO data reduction pipeline for HAWK-I 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).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1B92D27F63AADD6F46370195B071DEAE89D0852C2
SHA-256FEB09DDCD143CAB6B8E974186BC63E8D1107C0E2F52B5913BEA7451BE3149AF1