Result for 0D855BA8899D3617D60EB7E80804322A37971950

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-1.8.14/hawki_step_stats.la
FileSize1009
MD59F826BFFF24DA9AAA6CD7A044E379596
SHA-10D855BA8899D3617D60EB7E80804322A37971950
SHA-256FA8756E54984B4D1C94506E9BA25AA15F30F716AF5848EAD2B46CB618E572F6C
SSDEEP24:PpeShuWJ5bi3UUoxIK+Ahmfvi4deEvD2NGDe5/Aj6:b8WJksxIK1hmfKrOLcAO
TLSHT15111EF3F938E5226AFD00A554A8F303E46D9883C47271F5052CBD5DB614B51911AAE67
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
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