Result for 0A70E06838545EAABE54BC8F6771CDB19CED1869

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-1.8.21/hawki_sci_jitter.so
FileSize45832
MD5875C7B7D1B34F8F249EC1636F5D5CCD0
SHA-10A70E06838545EAABE54BC8F6771CDB19CED1869
SHA-25615C612BFC8708079E65BB48219D4B8F728EDB2BA80870B3A2E922A8FF3E8995D
SSDEEP768:nD9fLeuwRanbncPTAu3MIgoyOPrb73z9XPthRiBeHDt8hCjEkvoW6wPfjSe9uIqC:ZbwwlDWlsBHCQkvoW6wXw3
TLSHT13223D793EB542F57F2D1CE326C3EC171257CACB3730083839AAD84A459079DD8DA5A4B
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
FileSize216900
MD558F4C14FBDAB174013AEF2ADD25C1325
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-1FB0E3DEC94087E5EABFE6031DC01EEAB89A68165
SHA-256EBFA621F4DF309A4CFE2A32612DD9B29AB3DC5A9CA11F9F427CB74E87E4711C7