Result for 0E331396FD64C646C394EACC208E2ECBB9A21266

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_subtract_bkg.la
FileSize1047
MD57E50BAB491C7CFBE7BAD5A065939B73B
SHA-10E331396FD64C646C394EACC208E2ECBB9A21266
SHA-256A1FDCAE7D0F8ABCB8A94519C13C4DC7C49C42091CB99362DDB6A69CC65924198
SSDEEP24:1eSGWWJEOiw5xIY+Ahmfvi4HvD2NGDe5/Yxn:3GWWJc2xIY1hmfKQLcYx
TLSHT10211C03A83DB9125BAD40B5D8EDF703E429948790A2A5F1053C799DF128B43B2557E23
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
FileSize227748
MD5B2ACC305E3A6F4603A32574AC2FA46EC
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-1FAFAFF50844AC69EF126AC054E01E64C67733705
SHA-256129BF7506968CEB0DAF1299EEF863D41B29E5AA4EBA5505D0C3DBD8CAD911A64