Result for 0758D19E46F24A304638DA89FB6698789757130A

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_cal_dark.la
FileSize995
MD5A0EBACD959C08198722E193F9FD0683C
SHA-10758D19E46F24A304638DA89FB6698789757130A
SHA-256B7A617688D20C4B1BCCB06B0E88E5655DD3542CD8CFB4336341DA9CE23BB36A3
SSDEEP24:4eSG1bWJJ4ifTTLxIY+Ahmfvi4nEvD2NGDe5/B9p:UGVWJHDxIY1hmfKwOLcPp
TLSHT1C911C57F93899525AFD01A4657CE362EC2CD403C47160E5453C6DAEB114B5391266F37
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
FileSize441700
MD590A8B68481078A3E72CFC40CE28E0F8A
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-19C4376EABFD6588229052226F6F1AE0C1D40B920
SHA-256613F99F73A40908D157F4AE391FF2BBCE5911C50EC90D7A17D61089B608EA276