Result for 0871B950801A9E0DA5DF831677B4C95BB6C432B9

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/hawki-2.4.11/libcasu.la
FileSize946
MD59C69157669A32DAD234C0E727852038C
SHA-10871B950801A9E0DA5DF831677B4C95BB6C432B9
SHA-25689DE48295C2BA800139A78C8A58913079C989827CFE195E60D0F5C805B96F646
SSDEEP12:CZ4fWgxHY/r5WFKziJLiG0kLxIha+AAmBB7Szf77ixCF1VvT3RTZ/9IMCDwDqaAi:CWeSHOWpiyxIY+Ahmfvi4zvD2N0De5/8
TLSHT1E311E17AD3A94A367BF0095546CF306F826A403C97670D2441CB99CB324B82631C5FB2
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
FileSize494108
MD502A3A726877552855F37063639962D69
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
PackageVersion2.4.11+dfsg-1
SHA-1F0C3B24956A696442FCB32E293471A377BAA1960
SHA-256B278D9B2C829C63930C1DD03871AC2A331689C9689B54528681565BE256BB13C