Result for 28D77158A8C652340ACE41CBCA1DAD35B4F9F614

Query result

Key Value
FileName./usr/lib/powerpc-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_cal_flat.la
FileSize1002
MD5AA7C17C69F5A3CDA41EE629F9787DB3C
SHA-128D77158A8C652340ACE41CBCA1DAD35B4F9F614
SHA-256333278DBFB8FE944A547907D666ECC9CEE9EE77F53B8B326E6D2504DFAEC3399
SSDEEP24:okeSh+WJaciQO5O5/xIK+Ahmfvi4W0lvD2NGDe5/Oh:TAWJgoxIK1hmfKu5LcOh
TLSHT1A211253F83AA922567D00A574BDE323F42DD80384B170F1453DAD9DF114793A12A7EBA
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
FileSize184096
MD581950D6B382DAA6D7864B030252CD235
PackageDescriptionESO data reduction pipeline for HAWK-I 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
PackageVersion1.8.14+dfsg-2
SHA-13A7129DA572757788BD93ABECEE5431E938EB6C5
SHA-256F8F6FC29BA3956C3DCD876B690A995927917F6A0CE60DD48F42A86EE81F81362