Result for 0E7BBC1A05FF4CC9902C6871771AFBC47ACCA02F

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_cal_dark.so
FileSize22824
MD56264F2A9A668F98684E850BE0EED2A71
SHA-10E7BBC1A05FF4CC9902C6871771AFBC47ACCA02F
SHA-2568A502F90C96433DD81C9F635A892F97373EAA6F288D3AEB084B1543935D25070
SSDEEP384:XmnNGwm8b2ggTjNltlCH81DcYibgkDhv/jVyo0K8Zs8eFy2dyib1kC9CL:X2NGwpb2fTRlHCcWpbLDhzgtT+y2Qq
TLSHT15FA2E78AF95AC731E5D222F01A1B592AD9304400FA43D7227F8C2357652266CBF92F7F
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
FileSize260978
MD55F77ED0FB77CB9283D78B6CC956FBAC7
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
PackageVersion1.8.21+dfsg-1
SHA-13D00E429E99C1B8D428D87C587056182BBA9003D
SHA-256C39FAE0786F62BF2CDED8B18E826ADF7C549FC82B84F7602C5DC53034AF832DA