Result for 1F63ED59044D3341B6BF309B54F0D95BD0B384FE

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_util_stdstars.so
FileSize10624
MD5D1989BAEBD05F500676D44B2C2904EF2
SHA-11F63ED59044D3341B6BF309B54F0D95BD0B384FE
SHA-2567EE0C3C79B65B0C81912431924D9A8A53D922327A166D43EF2F72F356CFC1BB1
SSDEEP96:RWXkl+9BWBPJx7vwtQvz18VBj0t+jxAFhTjIZadxWUt8EB8Ueu+OZ5+iSjTA0nn:RW38p/vwtUz1C0t+jCPkaRletLxi
TLSHT12122C70AAB958A7FC9D49334406F473237B0A484DB2603373584B2353D527DC5A3BEAB
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
FileSize238384
MD5BD0858144B9991FC7E5BAE6A82F03021
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-18DF945A85ED8F9B9ED454AE4BF385B1504291ADF
SHA-256A63DB43EAB793C6B3E0BF690F6285C633FB2628F6470D923308272C4B5966746