Result for 0A3281AFEB1F17F3211745D591FF7BA652D9FB46

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_step_apply_dist.so
FileSize68520
MD52DFBD641A5C48DC213DBAA9B2C5CC6B6
SHA-10A3281AFEB1F17F3211745D591FF7BA652D9FB46
SHA-25635B1E0AAA0CCAE210E315676D1281209922622DAE75C746849EF263BBC73F7EB
SSDEEP96:gUQBWBrvXrco5Y9jyxiNDVBdiK4zUn7yFOEyFAxsNl4s8Px4VP/Lg67CL0GjEA+U:gv8toosBVB/YOzWi18Px+nPAWiF
TLSHT1B263524AB61CC82FC6C033380CEF0BA4B5738585F3569793345C51A8AF8C3A99B265CD
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