Result for 275A7445A19D67938D2B53F2D3E76DE85636B55C

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_cal_flat.so
FileSize45192
MD565F616DDED36EC35B57D7B1F38A87B9E
SHA-1275A7445A19D67938D2B53F2D3E76DE85636B55C
SHA-2569FE5EA96E5C5CB5D11C85F09E57F89495621882E2B6126B61D0A2DF3B9E7569A
SSDEEP768:3b6CG7lwChIMCXuk+by6YmUdKJ7V6O1PzJ:3+CwwXek+byfDdg117J
TLSHT1F813184FA4A05EB8C4E4A5349DEF2711B5347991F730DB5A120852B52E0277CE32EBAF
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
FileSize515728
MD5178BC39B67CCFAC7374837B6783DEFDE
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
PackageVersion2.4.3+dfsg-1
SHA-11B3779DC0D999F9AA02A89F5F799490440FB4A47
SHA-25688F0D4E52748D0A396F071C0EAF70FDD8F9BB0D1A987F7729A2B4E284A95C891