Result for 1AB80D4B35642FFB216C1F940EDAC7B9CCA24F0E

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_twilight_flat_combine.so
FileSize69464
MD5533853AACAA6FFFA5DC234D6AD206E59
SHA-11AB80D4B35642FFB216C1F940EDAC7B9CCA24F0E
SHA-25699D9953BD19AD777755373CC947F8EDAEEB7A087B5F453ED5AFD326628E7B5B0
SSDEEP384:fOQWPycC1c8snSDpB7qyxP6fU+rMKnNkWL0iaszp4xc614a5bAa4mtKW:fOQWqcmcRS1IyxP6jn0mzp4x1Ga1
TLSHT1F86397A3363C7B09CB10F439D5FE5620A3A16E4F97314603A85493272EED76C4726EA7
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