Result for 173F19803620B57DD3DF5059735088E8BB89FDD9

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_util_stdstars.so
FileSize68024
MD54154AF6B29C51BE1974BE34A38AD2C9D
SHA-1173F19803620B57DD3DF5059735088E8BB89FDD9
SHA-256F95FAAC13E1805046B50D0052E1C058AD8597B9E4E2662C312AFDCD3C2C92AE7
SSDEEP96:oeBWBix7kvZZPqjxUOeVGiSGcGFaxZZ2Ksnrj81oSFJ+AVj5dMo7v:n8GkvZZijxUOwGufAxZZyP81oSacF
TLSHT17D639593B32E5B5FDB14A63880FE577073A1AD0E43234B136504A3296EE976C8F61683
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