Result for 0554377EEAA83BA4C45B9E6D7F0FAF0527531040

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_cal_distortion.la
FileSize1031
MD57E15B44D91EEA9EDB6E6DB345EB55257
SHA-10554377EEAA83BA4C45B9E6D7F0FAF0527531040
SHA-256E83AD552636E797DFA889209069339498E90A5DE32E37AC8F7666A72BE771669
SSDEEP24:BeSG1bWJ2mioRxIY+Ahmfvi4J1vD2NGDe5/B9p:7GVWJowxIY1hmfKIpLcPp
TLSHT1CC11E23F83899176BFD10986468E362F429A407807512F5093C6DEDF174F839B267F22
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
FileSize441700
MD590A8B68481078A3E72CFC40CE28E0F8A
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1build1
SHA-19C4376EABFD6588229052226F6F1AE0C1D40B920
SHA-256613F99F73A40908D157F4AE391FF2BBCE5911C50EC90D7A17D61089B608EA276