Result for 03B93CB27DD400C50FBF5B267EC14FC6D41E9775

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_step_compute_bkg.so
FileSize69088
MD500553C72568412921E177D22368DA684
SHA-103B93CB27DD400C50FBF5B267EC14FC6D41E9775
SHA-2565EECE2A2C75612F3D9FBA43BA9A7D3341785AA01BB8E6C7C413FB8D161444063
SSDEEP384:zIPnT8WGoueU4Xwg2JYlvTCy5RQ1jk5MCPFTlirEDGLzig0yDP:cnIzoueU4graLC+oYOYT0EAT
TLSHT1F463B8A3366D9B0AD741B436D2BF163062522E0F43314B03999493366EDDBAC9B32D57
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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