Result for 1B65843C94A2AE1F91D6A441629E00FB089BA0FF

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-2.4.9/hawki_science_process.la
FileSize1040
MD5EDC59218FE7DB75BE01F99C19C5CF3EA
SHA-11B65843C94A2AE1F91D6A441629E00FB089BA0FF
SHA-25633B2549C738E2AC61FD9A5A6FAA1E097C9129E41921F9A4595B2AA5BB1F5CF0E
SSDEEP12:JxK4fWgxGb/r5WFKmx3LiBx1Q1QoxIha+AAmBB7Szf77ixCFltvT3RTZ/9IMCKbO:VeSG5WJ9iuxIY+Ahmfvi43vD2NGDe5/5
TLSHT11811F0B7C3CD993967D00945A6CE342F568AC4380B1D0A3492C6E5EB2A8742A1157E3F
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
FileSize432820
MD5C12CBBEF48D8105D146F3F56E4FC6A80
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-1E41BD0569D8F9C390A871D226FEBCF087EAA5725
SHA-2561645C1BA99874DEA41DB29C0692F68499585F6E8E7C1FA36686DA058B91EFAFC