Result for 10C79B7DEFFE8797C46DB979EF358919E196023B

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.14/hawki_cal_flat.so
FileSize27548
MD5285FEB6F90A0D432EE309C05D2635B82
SHA-110C79B7DEFFE8797C46DB979EF358919E196023B
SHA-256D2D55402F46C0135B201C316FF27336ADBE750B4A58DCDCED5C45E1F98ED5710
SSDEEP768:1b504iGHfXvn/3PHfMEcUsk80MEcUsk80MEcUsk8A/MEcUsk8091NFdVtl91NFdY:190sHfXvn/3PHfMEcUsk80MEcUsk80Mb
TLSHT1E1C229DE5AB79C23C4E2A53AA96F1F19009C55EDA61A4FC3295C40801603FBC957EF8F
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
FileSize220538
MD531D6CCA4666BB9CF91D70F85DF43457A
PackageDescriptionESO data reduction pipeline for HAWK-I 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
PackageVersion1.8.14+dfsg-2
SHA-1260CAF94A6F4CE159F52A9364FA6A81610CC3619
SHA-256A2E741FAF01616FAD42B2B5AE51B4AB0CAF93A19207EB47B6D178189F6DF71C3