Result for 02CBBEB49AE8F0C9384847455F95B01A15342B10

Query result

Key Value
FileName./usr/lib/mips64el-linux-gnuabi64/hawki-2.4.3/libcasu.so.0.0.0
FileSize198272
MD56C7B5E6F89551664166BEADE4F4FCB45
SHA-102CBBEB49AE8F0C9384847455F95B01A15342B10
SHA-2563494D4409CC704ED0D13F01055C627B80F23354EDF653578447A6A4AA3D3C426
SSDEEP3072:qWLS43P9GN8GD+Q9+ZGOKVrMdIBZm98NM8wuzA7foAq53c6DuaqXbPlDEZ/:/GN2sUGOUCIM8mF7hqn2DlDE
TLSHT11E1419969F482E87F1E1CF348C7AD272313DADE7B3108552DBED4D28690B6CB4E4254A
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
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