Result for 0F48D2CF9B14AE0932B699C9702F41BA64E66B3D

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_step_detect_obj.so
FileSize22744
MD57243980E1DC28919A8B4C45651ACE2A0
SHA-10F48D2CF9B14AE0932B699C9702F41BA64E66B3D
SHA-25634C7B127FA5736BB46BD9A34CED872BA854747891EDE829DC05F6DC4E37246E7
SSDEEP384:oxJhDjbiggTjNltlCH8BiOAJM6lLRwWJRJhMqgDcd:oxJh3bifTRlHCcBnAS6l++hDd
TLSHT109A2D44AE551DB70D5C73E7048530138AA729650F30FC7A3298CA75BA5A264CFE3E63B
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