Result for 17C13EE7A5AFB6037CECED74DDF20CCE034F4036

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_linearity_analyse.la
FileSize1043
MD56D9F920D83BDD503F4A4FE1EA555DDD9
SHA-117C13EE7A5AFB6037CECED74DDF20CCE034F4036
SHA-256D721243E11E8C90E33DD48A6CE2EA2D3F6CE7BB74D6D6159A7646D6FD13033FB
SSDEEP24:cDeSG1bWJe9iUXXKxIY+Ahmfvi4ybvD2NGDe5/jp:cRGVWJesUXXKxIY1hmfK/vLcjp
TLSHT1DD11203BA35915392BE40B4616CE346E47D9407983520A8C82CAA6DF31838693357E22
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
FileSize363444
MD5008665630BEAB04AA3E699DF53464A28
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1build1
SHA-1016893D9A8DABB8BCACD581CEE5327857904F01D
SHA-256C671E8C5D435484D7BD2ADE46FC2CAA48D49C8518AE118BED3AB6D604EE5336B