Result for 10102D9779FAC8A843D853B5389CBCD90FC96DC5

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/hawki-2.4.3/libcasu_catalogue.so.0.0.0
FileSize86424
MD53C9D5A258DEB37974EE719948028BB72
SHA-110102D9779FAC8A843D853B5389CBCD90FC96DC5
SHA-256FE6B8A465321027AF97F9E67C2BC580B6F56F4F776A0C5313008FF30117B6E0D
SSDEEP1536:mFuGgZtglJc5iuDoQ93LsSH22RoTVKSRJNFosalzDggY82XbT:kuGDHc57Dog3PqtRallS/
TLSHT15E839E8DFB8E2101C342E938B3A34F085AB8D59893765F8729D4C73C0723A595277AF9
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
FileSize471024
MD5948CB92838A4404E1AA12023641CDAB5
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
PackageVersion2.4.3+dfsg-1
SHA-12E3B1A4071995F103CF47F407CA4EF4591C36C9F
SHA-256382F8A1605747E26EE33758BD402E6C71DCB38950105E0EEF9E246951EF5205A