Result for 1C1C71FC16033E09A83D6A8A91D4C4A85E9511C6

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/hawki-2.2.0/libcasu_catalogue.so.0.0.0
FileSize98512
MD550BB99D595FBA4AC0F1AEC69B511A73A
SHA-11C1C71FC16033E09A83D6A8A91D4C4A85E9511C6
SHA-256C3343749809CB336FB2646778E072D61E6EC93EC18A01A4BD688CFCB00CD3544
SSDEEP1536:6F9hsQQEElEMu4pXQ1EYEOxzUTzKiyOTlpGEBjpbTq:Ans0sEMlCXQ+e5FpP
TLSHT16AA32986FE855A91CBD2E779B5BA138C313342E487BA314B8954C73C2FCB198A3275C5
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
FileSize353598
MD5A1BD40963DB2A77A0D7730FE85D0AF94
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1build1
SHA-1EB736B139332F6B26DE6CFF7CB6FC31819963E2A
SHA-25697C93587330F9AE975DB4E10FD12ADD6E9FA3078083991808F019B208598BCBD