Result for 089E00CF92A96D123FFA3B309F5F3284B3BDB367

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/cpl/plugins/hawki-2.4.3/hawki_step_refine_offsets.so
FileSize19920
MD5C20B4F24BE96BB571837C2975571CAB9
SHA-1089E00CF92A96D123FFA3B309F5F3284B3BDB367
SHA-2563AC3AFC4913CC8225886A1365D21C00512111917AB2BBCAAE39ACBA3457149DC
SSDEEP192:mFvoL/XCV8jnXA1YwtVnCTXuFka8rFgLvTxB+utqrs2h0jPf2ZQykiY0:mBoL/LXA1YwtVCTBaXqrQzf9t0
TLSHT1F1928397EB146E27D6D0CD35842FA5721E3C8C9BF3505383C94C81A05C0BE9C6EEAA5B
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
FileSize459464
MD5BF5AA2AF1FD8B5940C7561CD404DCF95
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
PackageVersion2.4.3+dfsg-1
SHA-1FBE7872286CE89B53E0544E3D1E8C86BB09581AB
SHA-256A6ECB0026D06870834397818D25A9044D0089E2CC575310F24458F40D0F1B52E