Result for 1B4A41AB48375AA83B691E28BDD25976CF1BCF9B

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_sci_jitter.so
FileSize69736
MD5B728CEF2489CA238AD65A8DD05BC365B
SHA-11B4A41AB48375AA83B691E28BDD25976CF1BCF9B
SHA-2569242E61658534A69E3295059BF3379AC2D87768A89D2124E090C21542E6F4377
SSDEEP768:YMM41deuwhXOejdYc1Uv8uWTkMAjYjIQQVwWr1VZt1TEfjSY9uIqP:Yy5wZ9ZqnW/dMvrPbpmC3
TLSHT1E863B6A3773D9F0ADB913435A26F09A061316D8396318603596883657FCDB2C9F3AE1F
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
FileSize224692
MD5D1343C262A1A7E0BD8BD4569E23F068D
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-15671A6932A008A7BDE978A313EC947BFE2999B20
SHA-256136A0A4E926B114E41A51F5D4B1915255A9E2B8943770353493F216FBD564D4E