Result for 2709221F623A05DCE17E417E6CAB458DC7136003

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/hawki-2.4.9/libcasu.so.0.0.0
FileSize199060
MD5B0FCFAF6BF9BF8A5519D110BC8C5D3D6
SHA-12709221F623A05DCE17E417E6CAB458DC7136003
SHA-256C508D076BEDF68243824D60CAE4364A2835FA8D57553AC8BEFF3A20A9EB9B9D8
SSDEEP3072:9FJEXb1WZXBUvh3FjvIHyvbygwHjqoyv0lWf4anAKitmpMIIADfGzdGHQ+dqYkN:Ib1ERUvr7pbXwHjqwwQanhpMIPvqYk
TLSHT1A314196CEBD2D4F0E0A311F04577531699340F25A23AF2E3FFCA3A81A971B95A539325
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
FileSize524536
MD53FC8B3C34A65DF11F4044DD0DED779E6
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-170C4037CF07C67D800F6A6916A4412B35AFD6356
SHA-256A4615C80DE8B1365075BBBC5B4DEDF45435016BCDC59F1DE203D83F86568C5FA