Result for 19AC7CEC231D66AE3BAAE698981910DC972D0A96

Query result

Key Value
FileNamehawki_util_gendist.so
FileSize18304
MD5B744B629D9274A34BF4A3CF4CD94FA94
RDS:package_id182052
SHA-119AC7CEC231D66AE3BAAE698981910DC972D0A96
SHA-256BB7FCDDBC574B30100D6FCC367BBA1C7A818111378D41153974D82F9A9BF59CD
SSDEEP384:adjBwE/MbrggTjNltlCjRDwx5Swb9ikX/qsZBMVO:adjBwE4rfTRlHCjRDQ99BSYMVO
TLSHT13082D84EFA83D7F2C1C672B82117063E6D708910F60BC3537AAD62C46652658FF6A739
insert-timestamp1679423153.2028959
sourceRDS.db
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
FileName13697
FileSize222964
MD5974C59296FB3D0C20D19308DD77F09D1
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
PackageVersion1.8.21+dfsg-1build1
RDS:package_id182052
SHA-14E0EAFAA7F8F95F0090AB88C11D17F77A12BCCFE
SHA-256266882D5AE449DE6BE617369A30F14C4281B4D1A395A3C0695B24BA38DAC0ADE
insert-timestamp1679408379.314181
sourceRDS.db