Result for 0120F540A7A9C52121BEBC92D866C0126EA40B8E

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_combine.so
FileSize23496
MD5A9156B275559D0B4C7750DE44A06D91A
SHA-10120F540A7A9C52121BEBC92D866C0126EA40B8E
SHA-256086A340E7A6A8DED523F9AA3C7AEFFA6B2944477D258D40A84C4CBE033BB774A
SSDEEP384:Si6TIycwPcaMdyKHQ61zp9D9e30/FovgKKrbbXPVAUH1qKrBcS/i/K/XbPN2+TLL:16TIycwPPMdyKHQ61zp9D9e30/KvgKKd
TLSHT100B2B6A3AF181F13D4D2EC34382F915250FF9E5D61989753E85DC8902A46AAC2DB7A0D
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