Result for 1210AA476C62C55D24CEF801E630C99878615739

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_util_stdstars.so
FileSize9844
MD559AC625A3BD1F4D1639FD393F79425D7
SHA-11210AA476C62C55D24CEF801E630C99878615739
SHA-256F0E1D55A82461B77DBE55796722817B15E3EBE094C9DECE399F3E9769025AFD1
SSDEEP192:My8GLUedpeBX3Qgc2EHx19Mjy9t07LQ5HU0voP8C:MsDmggKxPb07LQxU0gj
TLSHT12D12C74ABB86D8B3D2E911B8544BD63ED6308514E757C3A3350C23DC5C22B98DB223BA
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
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