Result for 063D72A24DA105248D96B36A1CBAD5733F5C3228

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_tec_filtchk.so
FileSize68080
MD5ADD55DC98468013C83CD4C2C375DF8DD
SHA-1063D72A24DA105248D96B36A1CBAD5733F5C3228
SHA-256B47A136712F526D9CE60A476DD75703CA249F341727BD15346570B5BE5F9DA67
SSDEEP96:hEdBWBUk3wpywTVRSm4UX8RtC3keVHLcFcKC/1dGjLYM58Hsf+ArW/EIccCHJV:A8GkxwTVdsDCUsrcaKCejLf59Gn
TLSHT13863639EFA98EC2FD4D4533488DB83F8B6B28404E3229F53750842647F0B7DD196798A
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
FileSize449624
MD5D0F643F072D886E3E40C2CF001467000
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
PackageVersion2.4.11+dfsg-1
SHA-1E4B3CF0B72CB879E436EB5436B6A298D1A1E625C
SHA-25661D5F2B79EAB5F4A393688ADD1495B2461504B353BE7F9EE0F9DE4C0CB4D4609