Result for 1A621F24FCEE97FA60675AFB06F46F46B9C6FE01

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-2.4.3/hawki_cal_dark.la
FileSize999
MD5AF814DE8EE5CDAAD385368A9A7F3AC21
SHA-11A621F24FCEE97FA60675AFB06F46F46B9C6FE01
SHA-256B1F0AE972A1BD6AEC2BB2385CC971E734081F8D8D83BEECFE115B1FEF349126D
SSDEEP24:4eSGsWJJ4ifTTLxIY+Ahmfvi4nEvD2NGDe5/H:UGsWJHDxIY1hmfKwOLcH
TLSHT12C11027FC38A9529BFD02A46578E392EC2CD803C07160E5453C6D6EB124B53D2266F22
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
FileSize459464
MD5BF5AA2AF1FD8B5940C7561CD404DCF95
PackageDescriptionESO 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).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.4.3+dfsg-1
SHA-1FBE7872286CE89B53E0544E3D1E8C86BB09581AB
SHA-256A6ECB0026D06870834397818D25A9044D0089E2CC575310F24458F40D0F1B52E