Result for 247FB5E78EB5154D276A8E8D41D14D39F73D2898

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.8/hawki_step_compute_bkg.la
FileSize1040
MD587552737E4A47EF61C0172B5602BD2E2
SHA-1247FB5E78EB5154D276A8E8D41D14D39F73D2898
SHA-2562CAB0B4DD31BE6A99B836432D0316EBB98B9B2B41EFDA006B276C8BE95E1D2C4
SSDEEP24:0ReSG5WJmyOicJJy5xIY+Ahmfvi4C1vD2NGDe5/Ajc:0LG5WJmmcJJwxIY1hmfK7pLcAQ
TLSHT16111E23AC3C95525ABE04596579F303F428B4C7C07276E6052C7D9FB114B81B3156E22
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
FileSize454368
MD560DE75C96E5EEC0B0CB809D3B38C05AD
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
PackageVersion2.4.8+dfsg-4
SHA-12362C669BEDA660467F4EAF89E0BD6020E351A71
SHA-256A6CE560A5A7EC6D78F19A88181F56DD7D73263A6DDB72A6C829DD442A9F575A1