Result for 06A917841C57F0786FEFA04E982844F11FD06749

Query result

Key Value
FileNamehawki_step_stats.la
FileSize1003
MD5F082668A4A8E3769234D1BE3349A5733
RDS:package_id182052
SHA-106A917841C57F0786FEFA04E982844F11FD06749
SHA-256FF873C5CE057BB451A3BAB3F0B4C8E3B54CE1210BBEB585614668C6BF4751B44
SSDEEP24:PpeSGWWJ5bi3UUoxIY+Ahmfvi4deEvD2NGDe5/oxn:bGWWJksxIY1hmfKrOLcox
TLSHT1B911023F938E5125AFD00E454A8F303E46C9843C07371F1052CBD5DB614B41A21AAE37
insert-timestamp1679423153.1895845
sourceRDS.db
hashlookup:parent-total2
hashlookup:trust60

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Parents (Total: 2)

The searched file hash is included in 2 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
Key Value
FileSize260978
MD55F77ED0FB77CB9283D78B6CC956FBAC7
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-13D00E429E99C1B8D428D87C587056182BBA9003D
SHA-256C39FAE0786F62BF2CDED8B18E826ADF7C549FC82B84F7602C5DC53034AF832DA