Result for 025CCBDA3F9A57D30E91555143C809CD74ACEF2E

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_science_process.so
FileSize91192
MD58717FD6B942B40CE1104A727EA356C3A
SHA-1025CCBDA3F9A57D30E91555143C809CD74ACEF2E
SHA-25699C444CD45C367DD0C1267DADD8573440A318A11EFA4D86D81E7ECF7CE1A96BD
SSDEEP1536:QEp8LuDjXnIoMjJFjgv4hTAuEFAzlb1SO9W:1qgkf7YGaelbY
TLSHT1BF93E747B69149F9C1D0D631DEDF51239630BCC0D634B32F7884A6262F117AC9B6EBA2
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
FileSize489816
MD50DC386B9AA2A31F951B2CAB6994240A4
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
PackageVersion2.4.9+dfsg-1
SHA-1174D5C4F5AF18807F53EFF58FA4460491B0A01A0
SHA-2561A2BE31E56411C85A56DFA78B4D7E21032BB44C3A3A3C03F2A8F1F1DD66465F1