Result for 0ABF889197DD47129B6437D9B955BF565E71A0E3

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/hawki-1.8.14/libhawki.la
FileSize955
MD5963A1E3744F67E126C7EAECE35D5F750
SHA-10ABF889197DD47129B6437D9B955BF565E71A0E3
SHA-256E6F07EAD23082D3AF5261268425BC91C083AF8E506478CF5A73BD3EFA33563D1
SSDEEP12:o4fWgxh4/r5WFKiJLiORxI3a+AAmBB7Szf77ixCFlvT3RTZ/9IMCDwDqaAlH/HHg:jeShuWPimxIK+Ahmfvi4lvD2N0De5/g
TLSHT1E411E13BC38A463677E046554BDF302F835E843947570D1052CB99CB234381A31E5F72
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
FileSize235558
MD5B07F1716E526AC3171FDD3D19B6361F7
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).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1FF4A18E1FFAB4BD4D31FE1BE2C866401316953B6
SHA-256FF0CE99CD7E6398A4E477532FD9D5B3A7D05EA786069F1522624BC3E1B406AAA