Result for 06CF36F534CD5283FB8EE1E95BA756C3DF4CF474

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-1.8.21/hawki_cal_distortion.so
FileSize28480
MD5791708BE4C1DD4A701F9AD51509323B3
SHA-106CF36F534CD5283FB8EE1E95BA756C3DF4CF474
SHA-2565958DABAA9CA12FBE9131E05591136A7B376986ECA3D96FF5B6A8461D6434131
SSDEEP384:Hnml8sw/xTVVkcgtXV+kElzqDGpe5hsce:Hnml8swZT/kltXVylHpL
TLSHT1AAD2B4A79B557E27D5C1DE33D42E80310A3CAC6B734097839D4E45E85E0EADC8EE6A07
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
FileSize216900
MD558F4C14FBDAB174013AEF2ADD25C1325
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-1FB0E3DEC94087E5EABFE6031DC01EEAB89A68165
SHA-256EBFA621F4DF309A4CFE2A32612DD9B29AB3DC5A9CA11F9F427CB74E87E4711C7