Result for 0F438E0738FAE22A308963152EB167F2F086A6E7

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.14/hawki_sci_jitter.so
FileSize31736
MD571FE839C1FD849CD360E3B7431D2D95A
SHA-10F438E0738FAE22A308963152EB167F2F086A6E7
SHA-2566AEC3EA8959DF31039ECA934DC0AB082F5769EFDB5D54B10CFF8E605DF49DF5A
SSDEEP768:LCRu3F/Zhpx5BJRZhpxmO2eGuW+mO2eGuW+mO2eGuW+mOeNeGuW+/HPXfnv3/HP1:uUF/Zhpx5BJRZhpxmO2eGuW+mO2eGuWw
TLSHT1D0E2F8D2AAF34917C2D56577A00F1ED9559CF4D2A219CF1F338C40A095026AEF63EE8B
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