Result for 1E8103BE39DC7989B848A10E368C68811ED7A956

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_cal_distortion.so
FileSize69136
MD5DD9D4A8A04EF8EB6A8143E6A5E3FA1CF
SHA-11E8103BE39DC7989B848A10E368C68811ED7A956
SHA-25684DAAE478FEF8F507174AE0008CF95C0B4CB43B701A1B8687B4286E44304C0FC
SSDEEP384:5I6IBJ8+CXLmOmrMjKAXzRIS+DycYcK4ZhflmxoDhRV+e5hscwqd+:0J8+6LmOWEK0IS+e0ZllvRUkd+
TLSHT1616385B3322D670ACF51A139A2BE563061A13E0B473047039D58D36A2FAD76DDB33A57
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