Result for 18952DDFED78BCB1FB259362695BA7909C6C7B64

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_step_subtract_bkg.so
FileSize68504
MD5D814ACC394E9C2E49D87AEE53C4C6556
SHA-118952DDFED78BCB1FB259362695BA7909C6C7B64
SHA-25644C3B07BCB26A70586252D487C2F85D8B8A8D5320D57AE8AD5DABC9E6B63693B
SSDEEP192:Ua8DWhQVBEhi0BobB6VAAe9QK5xgyg+ZM3J:SWhmCEIu0v2QM+yg13
TLSHT1C263614BB69DD82ED4C9633D48DB03A6B673850697129B83624841B83F097FE0D379CE
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