Result for 0AF7552ED81108D7C933250E63B372E41A61F9E3

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_step_combine.so
FileSize24128
MD5BDB4B150D84465AD2550A7F4B0B8B039
SHA-10AF7552ED81108D7C933250E63B372E41A61F9E3
SHA-256775BC29A535FFC5391F7E058A96B02616E15D6B6D6ED2D00E20B77665F44246D
SSDEEP384:0C/bwYwAN+qv/YwP4On6DLLE3XT4wmZ8aJfbT+czlU:0C/bwYx0kgQ4nDHjs2f
TLSHT137B2099B665267B6C4E4A334A0CB12252970FDD0F730D32F658811706D4276CAB2FBAF
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
FileSize479446
MD505163626569370830CB4BA3492E0B092
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
PackageVersion2.2.0+dfsg-1+b1
SHA-1CEDE6337214FC45AF5F212D7F8B8F84CD8EDCD55
SHA-25689D9D055F1AB77CD76E039FA4BC12C013BD5702025C1FA292279C2316B1D1BB8