Result for 0ADD5D841895384D6D3806F6D7F4DF3814D7F710

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_stats.so
FileSize10776
MD5338B6B82AD42F09E9E0F22FAEBCD5D02
SHA-10ADD5D841895384D6D3806F6D7F4DF3814D7F710
SHA-25644E4DB773C3A5C206594CAF30C76F6909AA4BBAE8C857E33A98B768455C1A526
SSDEEP192:HXE+d8b9w473jgvRwZYObA5+gFV81VpgJ6m+LAwbNvYZNJGkCGu0joP0Ixy6SXjF:He9w4zjiRwZYObA5+gFV81VpgJ6m+Lts
TLSHT166229727FBA91E22CCC4EC30091F472A55FDDD0EA755B723A40D81C06A057AC5EB7A6E
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
FileSize477952
MD53CAA106DD6246DCF218DE138AE022F77
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
PackageVersion2.4.3+dfsg-1
SHA-107D5C627FC555F637353012D04FEE7C6F1E6113C
SHA-2564B04179EDF606ECC3AE590EC5EB34589B088566F820C6F00530B40016D5D6193