Result for 08A0B3ECEFA7D1B5788DDAA19CF75C11BF751076

Query result

Key Value
FileName./usr/lib/s390x-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_combine.la
FileSize1015
MD5D0087F1EE98A910D643DF13A17F43BCD
SHA-108A0B3ECEFA7D1B5788DDAA19CF75C11BF751076
SHA-2560D242A72F597044F6BCAE2FC988BC3639F22C50EE90E1F08271CA1B36FA8386A
SSDEEP24:LeSGsWJ2Ois5xIY+Ahmfvi4dvD2NGDe5/j0:pGsWJiSxIY1hmfKALcj0
TLSHT16011EF3A939E6129EFE00A45968F313F438A8C7907212E6093C7D5FB114B8192166E37
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
FileSize468408
MD5AFB8672F4237B6E084ADD1D7965FEC77
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-15F5A26B6ED1A94FCCDB5418A6EA9D38509C7832D
SHA-256A8BF33C01629FEB6CE296AB321AF3C889D6452D6BE48DD6507E7D949D35B2061