Result for 1B9DE2F9826ED9C95FF637D1697BA73954D848C5

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/hawki-2.4.9/libhawki.la
FileSize957
MD56CA3C88E69D5C2AE3357F8F0CB4840A9
SHA-11B9DE2F9826ED9C95FF637D1697BA73954D848C5
SHA-2565591FE2F753E2D23DEB31D3FE98E246C27E634AAF1A4C74D1021C64A87036E7E
SSDEEP12:o4fWgxGb/r5WFKiJLiORxIha+AAmBB7Szf77ixCFlvT3RTZ/9IMCDwDqaAlH/MAv:jeSG5WPimxIY+Ahmfvi4lvD2N0De5/Bv
TLSHT10711ED3AC38A063A7BE04A559ADF312F834E403807670E2052CADDCB234382A31A5F72
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
FileSize525508
MD502A40EB100388240DB4D5D6169497C90
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
PackageVersion2.4.9+dfsg-1
SHA-11DF42B5AAC2B9A9BD2D43985F3D8ABB2D7B93FBB
SHA-25654DC6921752833B0AD602101C2BD1ADE309304A73249C9EFE3E22121EB856F01