Result for 30D89D09B9F693155366D4474CD5EE7AFF94B5A0

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.8/hawki_step_refine_offsets.so
FileSize18772
MD5709F58581389E19AB7341A7889ED2962
SHA-130D89D09B9F693155366D4474CD5EE7AFF94B5A0
SHA-256756E344E4998B97DEBFFEC4D51219C2F96B9AC4C237D1C4E2D8C2D02414A1593
SSDEEP192:biBao8jnXAlCiZ5+zUxtwPvGYFkdhlraMU34qlcIgs/LfbcVkp4c1qrpzLjfLx/b:biELXAlCiBx6GrOgKLfUkp4x3DLE
TLSHT1A582C6CFDE22CA67C9C13A34B12F4A54122242EEE3497B835B4845942E1775F9F62B4F
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
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