Result for 12C05A9269472E538DE548C61F29486C5D6E2634

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.8/hawki_cal_dark.la
FileSize992
MD57C097E73C6A2AF7A98F922FFFA25AD9E
SHA-112C05A9269472E538DE548C61F29486C5D6E2634
SHA-256EC310B2F3F0C09FC44B16627146D2F58D100E10355C43FED16F6E8845EF8ED31
SSDEEP24:4eSG5WJJ4ifTTLxIY+Ahmfvi4nEvD2NGDe5/Ajc:UG5WJHDxIY1hmfKwOLcAQ
TLSHT1C911027FC38A9526AFD01A57679E3A2E82CE403C07160E5853C6D6EB114B53E2266F22
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
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