Result for 18A40007C10794A4A5726FFD145303BAAC74F451

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_step_stitch.so
FileSize14728
MD5386C54EB29110A920F77FC3D39DEB583
SHA-118A40007C10794A4A5726FFD145303BAAC74F451
SHA-2561775081C085B5EF752439D629D286A09EF5991DCC8CDCCBC8C55637A5A824FB0
SSDEEP96:j008OatFBWBf1fzquJu5z1gSTj7u9CoJB5wSF3O0TF7+gGL1vJlE7/NgfH6w+AVU:XaD8LvuLp77oJZc1m/ufH63Zu
TLSHT15E6272AFAF3A8DD6C5E43B34429F837897798D24730947123BAC83141B577948E35A93
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