Result for 2F71E04DBA0450024837D8F1441CE239AD0B4664

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_cal_flat.la
FileSize992
MD5CB624DD83823C6055859357C4B1F46AE
SHA-12F71E04DBA0450024837D8F1441CE239AD0B4664
SHA-2561CB3DDD034FA0AF2ABACA7F5AD37C0DB8CAA50252724B915C98B35810EE273F7
SSDEEP24:okeSGsWJaciQO5O5/xIY+Ahmfvi4W0lvD2NGDe5/Y0:TGsWJgoxIY1hmfKu5LcY0
TLSHT1A111023E939A91296BD00A464A9E322E42CD40380B130F5053D6D5DF114793921A7F76
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
FileSize477952
MD53CAA106DD6246DCF218DE138AE022F77
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-107D5C627FC555F637353012D04FEE7C6F1E6113C
SHA-2564B04179EDF606ECC3AE590EC5EB34589B088566F820C6F00530B40016D5D6193