Result for 06ED73E9B68B9E89F0609F858530EC29EF5CB21D

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.3/hawki_dark_combine.so
FileSize18924
MD551068158BF329E59DAC3184E75E3BBB0
SHA-106ED73E9B68B9E89F0609F858530EC29EF5CB21D
SHA-25610B04A10B2BDF78A6F4EA37CB48B4EAD5ED337D964E0A11747E4358586E36B36
SSDEEP192:rr5KFVPaEE8RSPNsFF9tw8SzJzKuXAW8UwYtDzfv8vN8y7EsgewU4ov8A+p8XOlU:QnPaheFfwloXY35zfv8yy0yY
TLSHT15682D8C2571ADDC3C9C9B934347F8E1A56A5D2D8D5184B83318C046017D2F9F8A2AFAF
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize471024
MD5948CB92838A4404E1AA12023641CDAB5
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
PackageVersion2.4.3+dfsg-1
SHA-12E3B1A4071995F103CF47F407CA4EF4591C36C9F
SHA-256382F8A1605747E26EE33758BD402E6C71DCB38950105E0EEF9E246951EF5205A