Result for 0B071842879583C5262AC3350F8DBF0B78A6C974

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_util_stdstars.so
FileSize67728
MD501519BD8C7BECD7CE13CFC9F1CFE68E9
SHA-10B071842879583C5262AC3350F8DBF0B78A6C974
SHA-256827324E57EB10FA5CA1F602230CFE93B59DFB6B06D2549B22EFDC5A63ABD338B
SSDEEP96:rlDUSJ3xBWBPJx7vwt+2OLTpXrTiebx3Nvt5XsfKXajLR+RWtn/s:uS8p/vwt+2OLTpXasx3NVKng
TLSHT1F06371A3B72E9A5FC7D4263991EE43707331AE8603534313561453297FCABBC8E29A46
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
FileSize224692
MD5D1343C262A1A7E0BD8BD4569E23F068D
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
PackageVersion1.8.21+dfsg-1
SHA-15671A6932A008A7BDE978A313EC947BFE2999B20
SHA-256136A0A4E926B114E41A51F5D4B1915255A9E2B8943770353493F216FBD564D4E