Result for 08141E1A2122F7230B0D7D08DC38388AF7B5F70C

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_sci_jitter.so
FileSize45496
MD5F8DAAE8D9DDCC0AFC69A151CA663E1C7
SHA-108141E1A2122F7230B0D7D08DC38388AF7B5F70C
SHA-256ADAFB53C57998C901AD9C42A7C0EDA20D46D2CF6D1B4E2C3791212B07989A44D
SSDEEP768:1iDGwZKQdfmVs8NECmdNCBFqjtNuoYfn02gK69uIqP:8awvGs8N+dWgrul02gKJ3
TLSHT10D13198BB6619EB6C5E0A630A8DF13126530BD52F634D70B124C53711E027ACD73BBAB
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
FileSize494108
MD502A3A726877552855F37063639962D69
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
PackageVersion2.4.11+dfsg-1
SHA-1F0C3B24956A696442FCB32E293471A377BAA1960
SHA-256B278D9B2C829C63930C1DD03871AC2A331689C9689B54528681565BE256BB13C