Result for 04EA24D7F016579CF34D5E6D6B18657A2A1DCCCE

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/hawki-1.8.14/libhawki.la
FileSize963
MD51234CEC4F9726F01E83768EF1F4681C5
SHA-104EA24D7F016579CF34D5E6D6B18657A2A1DCCCE
SHA-2560A160616FF8A77B11FCA0A37E8BAEF20FD4117CA31F9A70EBAB3EC0AE9400420
SSDEEP12:o4fWgxho/r5WFKiJLiORxI3a+AAmBB7Szf77ixCFlvT3RTZ/9IMCDwDqaAlH/rHg:jeSh+WPimxIK+Ahmfvi4lvD2N0De5/U
TLSHT16211CB3A839A463A7BE046554BDF302E839E8439476B0D1052CB89CB234382A21A9E72
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
FileSize165216
MD5E12BAB3979675ED66624430A2F31F9B7
PackageDescriptionESO data reduction pipeline for HAWK-I 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
PackageVersion1.8.14+dfsg-2
SHA-14A0285D01B6819014CE86C3B6D1123F6534E36C5
SHA-2564F99F67FCA1A126F63922C859CAC6A04492F38E7C20EEF6402A54CC39E32AB46