Result for 28422DF49F9D7022D52F7D6B1702CE5770A3FD7C

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.14/hawki_step_detect_obj.la
FileSize1046
MD51DC4564A23D2BAB3B23938B7BC0038E1
SHA-128422DF49F9D7022D52F7D6B1702CE5770A3FD7C
SHA-256F26129B8EDE075117A28C78FB7A7E17344BCC45429BDD1C6D138996743E2B885
SSDEEP24:PeSh+WJU2icBxIK+Ahmfvi45vD2NGDe5/Aj6:lAWJUzcBxIK1hmfKqLcAO
TLSHT1E211DD3BD39E723AAFD415458ACF303E4299887947352E5063C785DB224B81911A7E67
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
FileSize182644
MD5B913E5F643EB90DB738980D1B4AAD78B
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1FA7B88CE6E858920EE04E01091AEADABC91BEEE8
SHA-256D9CB21642275832CBB1599E32BE54633E9B29C8FFD3316B6EE9E95706D7E4F26