Result for 21E9CEBE3BCFD55CA95475A7A02C4A3EC7C58C59

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.9/hawki_standard_process.so
FileSize44232
MD512B2EC70E0C14BF19C4E6471D7627AFA
SHA-121E9CEBE3BCFD55CA95475A7A02C4A3EC7C58C59
SHA-2568D90A2F742AD103A24FC3558FB3ABF6AC746819363481E8216B852EE49C82950
SSDEEP768:uQHR2VEcE4R7JaR9mB7CUDksEmTeKSTPONFO+lO+VhBJjg:VHR2VEP4/A8GU4sEmTVS7ONFO+lO+3
TLSHT1A8131ACBA8A759E3C5C4553435DECA68732286B4C3DA7703951CC2286EB22DF4925F8F
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
FileSize453352
MD55CFC0CB5C37652E14DA39B16073327E6
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-109AD28C108CC2A32C4F9E9E6E17CB27DA90FFD5E
SHA-2567A78D83C1E6E73EB9D53CA7D68B3C5EB49076AFE08652C402C0E2888B970DE64