Result for 11747B1616B998ECB3339E1B2901B3C517061A1F

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-1.8.21/hawki_cal_dark.la
FileSize994
MD53BC3DBCFE654BD1109569C9EFE2E691A
SHA-111747B1616B998ECB3339E1B2901B3C517061A1F
SHA-25676BE4441D7CDF9C2C985D35BC60AE9C7C1F6083E765BAD24D500080A7E2CA6AF
SSDEEP24:4eSGWWJJ4ifTTLxIY+Ahmfvi4nEvD2NGDe5/Ajsn:UGWWJHDxIY1hmfKwOLcAA
TLSHT19911027FC38A9126AFD01A476B8E392E82CD803C07160E5853C6D6EB114B53A2256E22
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
FileSize228074
MD5CE29F2691A6DA88FF83D73C679596827
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
PackageVersion1.8.21+dfsg-1
SHA-1FFAB13A4EB060F369871AD9885635F1D6BDEAB73
SHA-2568D0D52E213F4C1B1787D5035FF57338A5A51EE8C5F408362A01B3492A2590DA5