Result for 1F5B9CF04D84990A5B6011D03B14EDB92949FE37

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_step_subtract_bkg.la
FileSize1056
MD5D6E14B3F5288BCBF7E9D60A3D2EF4F84
SHA-11F5B9CF04D84990A5B6011D03B14EDB92949FE37
SHA-256166A8D6F45262673590AEF5F886291C498897D27A560AF4387DB2885C9A82303
SSDEEP24:1eSh+WJEOiw5xIK+Ahmfvi4HvD2NGDe5/vh:3AWJc2xIK1hmfKQLcvh
TLSHT15711233683D79115BAD4075D8FCF703E429948790A2A5F0043C795DF128B4371157E23
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
FileSize165216
MD5E12BAB3979675ED66624430A2F31F9B7
PackageDescriptionESO data reduction pipeline for HAWK-I 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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-14A0285D01B6819014CE86C3B6D1123F6534E36C5
SHA-2564F99F67FCA1A126F63922C859CAC6A04492F38E7C20EEF6402A54CC39E32AB46