Result for 23F57B0FD776DFED853FC56CA4EE56DA347EDDA2

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_science_process.la
FileSize1030
MD52E848396A1F9A01E068466CAB9686C17
SHA-123F57B0FD776DFED853FC56CA4EE56DA347EDDA2
SHA-256250118F6EF1C14D8432AD0012FFAA04F10BB600B7132F8C3575737CB3B7FCD2A
SSDEEP24:VeSG1bWJ9iuxIY+Ahmfvi43vD2NGDe5/op:XGVWJsuxIY1hmfKILcop
TLSHT1F211C0BAC3CD993567D00A45A6CE342F56CA84380B190A7492C6E5EB7A8742A1157E3F
hashlookup:parent-total2
hashlookup:trust60

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Parents (Total: 2)

The searched file hash is included in 2 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize438120
MD5F14E612CDAC168854029D313E0FF1BC8
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1build1
SHA-125C318905E702AE7B4F69DF645F83D37B0452B9E
SHA-256F63148016DA1AE247452781483A4BC1347D39621941BC5D9B51B2F5CE00EB9CD
Key Value
FileSize510596
MD5C3A8598255D089A56D7555D54E939763
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
PackageVersion2.2.0+dfsg-1+b1
SHA-126EC7B533367155E98EE1068CED505920F9DD102
SHA-256AE2F773418C6EAFE9CB8230F334D27A87C21AD03F9D91B92A96859FA35E55D2F