Result for 201614A5F4D3AC206941698BFECDAF73A468CCD8

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_linearity_analyse.so
FileSize26796
MD5D3FB4545FA989AF45CB6DEA45DDA45E5
SHA-1201614A5F4D3AC206941698BFECDAF73A468CCD8
SHA-256B627621A74CD3C998227EC08B614642E7479B93712B57E8E8F8F53A29A16710C
SSDEEP768:ECUHkwKGefTRlHCcRRae3b3Nwm85bJMMoYa:E2wKFtX/3ObJMMoh
TLSHT1ACC2A79FEAA1DC70D1D296B820273125D874C810B7E683C2FF4D3395AB11659DB3E62E
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
FileSize510596
MD5C3A8598255D089A56D7555D54E939763
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-126EC7B533367155E98EE1068CED505920F9DD102
SHA-256AE2F773418C6EAFE9CB8230F334D27A87C21AD03F9D91B92A96859FA35E55D2F