Result for 016E26BF89DC187551C549C1E56E21CAAAD9120B

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_cal_dark.so
FileSize22796
MD55E52D0060B31EDCC9228A1EF13D32BA7
SHA-1016E26BF89DC187551C549C1E56E21CAAAD9120B
SHA-25662B09221B0A479FA8FC64A95674E80CAC32BC310C21FB87FD23839676B583F07
SSDEEP384:XNCwlHbVggTjNltlCH8f3iGJpfckprFkhOUuAelNjjwGG7pOYyiWj8L+L:XNCwlbVfTRlHCcf3xBjtxAIV/TB8L
TLSHT1C4A2D7CAF452C7F2D1D271F4251B1B2EAD308500F607C7223A5D32D660D2AACBF65B6A
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