Result for 2379E8EEE537AF3049BAE03FD4D56F74667510B0

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.4.9/hawki_dark_combine.so
FileSize19044
MD5C1F360050D540F9D21EEC3B48ED411E4
SHA-12379E8EEE537AF3049BAE03FD4D56F74667510B0
SHA-25659DB7870AEC03E9219ED5DDD998C2E5B5540E26ABE8FA8576C6F031F1A7D4231
SSDEEP192:GLLei8eSPNsFIpSY4JQm2MU7cuFgtx0DSA2hsBu6ciWOfjnUq+lWPQZvqC3M4ovc:GLL4eIgPQmXUM02ha3uUPQZf3dJnt
TLSHT17A8273C3B64ADD62C8D1B63474AB8F42552582F4ED480B83319C0C665F02F9EC969FDE
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
FileSize448916
MD515510D708B30FD3447AB413D215ADBF9
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
PackageVersion2.4.9+dfsg-1
SHA-1617C0F0EC2D7EA25558AFB56BCCB07552925D079
SHA-2569202A8FDCCDB13C2F3ACC2DC6A1BDFA123AD464F752FF6FE14DB8FC365CA9AE6