Result for 0431D43C5E9FD738BE53B125B129BF72685B2987

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_util_stdstars.so
FileSize67744
MD5C9A9E1C2C55591666F3C92A52979A262
SHA-10431D43C5E9FD738BE53B125B129BF72685B2987
SHA-256D8CF4D6D818642E23F3E1C06535466711DD1B02DE4A7AD2987AA23F74D9E08BC
SSDEEP96:29lDU4BWBPJx7jx2+z+py2Zi+DlkvoeIIPPKXaj7KQ2+R8MttnE:2048p/jx2+z+pyZ2kBIYXvVmM
TLSHT142634063B36E9A5FDBC0263995DE43707331AE82035347139614533A3FCA7BC8E2995A
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
FileSize190308
MD54A9C354B9047366270BE90C85A9082F1
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
PackageVersion1.8.21+dfsg-1build1
SHA-1255B34E4F87A4AB7107B747E7A67F6995239722E
SHA-256BB9CA8E6CCCE01596EB08FC791C6ECDF3554D3E2D18DC55330F7EDA7CAC17BBF