Result for 1116D3DF5BDFC81E4393F673030FFFB535627DC3

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_subtract_bkg.la
FileSize1046
MD5964A1614630895B3A5EDDDA36F95350B
SHA-11116D3DF5BDFC81E4393F673030FFFB535627DC3
SHA-2569182CB7A3BEDEF348108CC8C3C1D86B183D896F696B77A3F404623ECE122C171
SSDEEP24:1eSG5WJEOiw5xIY+Ahmfvi4HvD2NGDe5/vS:3G5WJc2xIY1hmfKQLcvS
TLSHT13D11203A83DB8125BBD40B5D8ADF303E429948790B2A4F1043C798DF128B43B1557E23
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
FileSize446980
MD516EFB69819EAF8E09B64CBD57CC67A9B
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
PackageVersion2.4.9+dfsg-1
SHA-1BAF855C0E5F8829D60769AF9482EFE8ED23EFB36
SHA-2560E43A15CEC1735CDE3AE4C7FF1A00C540392D2A763450F033F2AB8EAEB957702