Result for 027C1BB4CBECA1EACB8B65DBCEFB3CD9BAFB4955

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.11/hawki_util_gendist.so
FileSize67520
MD552817CE799DEE50F71C4AAC206772791
SHA-1027C1BB4CBECA1EACB8B65DBCEFB3CD9BAFB4955
SHA-25641C32A78D452BAB64773074EA9519666C7742B393A2544A4D3589738E0B755D6
SSDEEP192:ncinz+8UOTgxs2KlIiwXQkgIk638k6kAtGFLWCUZMv5XvFC2aC:ciaCgxs6iwXWIx6kAtGt3UZQt1aC
TLSHT1F263B5EBEBDB2F9BC5CC6F70040F1F1617218AE9931AAB63184C4174090D6ACF65AF85
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
FileSize451432
MD5806CB6A07D053F721A8E675196114EB6
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
PackageVersion2.4.11+dfsg-1
SHA-1D4EE6BE1F295CE3F05E675E4F234B3A20BF3B199
SHA-256E2F48D24F4D2E931655F871957B4718228B438460887A47BEAC55B6C6D323744