Result for 108CC43E8604E033381D15A9A9FA25283868D492

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_photom_2mass.la
FileSize1045
MD581532904FA989A1B28E78E5B3F0D467E
SHA-1108CC43E8604E033381D15A9A9FA25283868D492
SHA-256D2597F31D17E00664FCB41411B33B58D918D15ED0F0C66DB8DD10E2D474E2AA7
SSDEEP24:ueSG5WJNmifRxIY+Ahmfvi4qvD2NGDe5/bS:mG5WJNZxIY1hmfKPLcbS
TLSHT10A11123B83995529ABE409465A8F747F43894539077D2E1452CB84EF124B42932A6E32
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