Result for 00B4A4D7CEC964816CEB7DE959C138F8D573B13A

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-1.8.21/hawki_tec_filtchk.la
FileSize1018
MD58136B729C4ACB0D5A65E3F0BB84D71C1
SHA-100B4A4D7CEC964816CEB7DE959C138F8D573B13A
SHA-256CADA936FAEC7B2E4237C0BE00305FB50B3FB230B54B3C611E079A67A21A4E684
SSDEEP24:NeSGWWJpiOxIY+Ahmfvi4rvD2NGDe5/An:fGWWJQOxIY1hmfKoLcA
TLSHT15C11EF3AC3CA7A297BD00E458A8F302F4689803C17250E1863D7A5CB5347C1A21A7EA2
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