Result for 222E733056BAF64065ADC61353CA50D674580753

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_util_gendist.la
FileSize1013
MD5967BEF864A25AA56333EE9688BF7D4FA
SHA-1222E733056BAF64065ADC61353CA50D674580753
SHA-2567A5E65EDD314EBCBD322E5D6A057BBFA11282C5EE09096BF4698E26969DDCF22
SSDEEP24:KXeSG5WJYZiirr2xIY+Ahmfvi48d1vD2NGDe5/oS:K9G5WJYAirr2xIY1hmfKvdpLcoS
TLSHT18E11EF7E939E612AA7D80AC5968E3A3F438A4038072D0E5852F6E5DB154F46D21A7F22
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