Result for 00D2FC7EFC6E46601767EDA578D952FF3FF3E9B8

Query result

Key Value
FileName./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_cal_zpoint.so
FileSize39816
MD5390F6C29F5072870162BDE14B3C936B3
SHA-100D2FC7EFC6E46601767EDA578D952FF3FF3E9B8
SHA-256DD12BD5007842037B5A722181F107EE7FA26778655E6B42956C7CACCD8382A71
SSDEEP768:gKFg/J2TwAg4G20+k2qk1jjqCwn0aE9TFIesAhn0a0P+7Q+Mre6D6QMvL2zUvf8a:2JmwAtGfH271jjqCwn0aE9TFIesAhn00
TLSHT1D803D4A7AF285F93DAD3DDB07C1E4282E0BE5D2CA19CF693F84CC5C03605A195CA3949
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize227748
MD5B2ACC305E3A6F4603A32574AC2FA46EC
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-1FAFAFF50844AC69EF126AC054E01E64C67733705
SHA-256129BF7506968CEB0DAF1299EEF863D41B29E5AA4EBA5505D0C3DBD8CAD911A64