Result for 24E1212EB04AEC3D982E72A9BF5BAEC4E7ED1207

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_cal_zpoint.la
FileSize1004
MD5A2E141A960922DAD4D554878177B79F5
SHA-124E1212EB04AEC3D982E72A9BF5BAEC4E7ED1207
SHA-2568D6EDD9A5627595871DB47F4A4C9B917DC2F7EC57C4DFECB7392E4166F6DF7E4
SSDEEP24:4eSHOWJ+izxIY+Ahmfvi4IvD2NGDe5/v1:UuWJ7zxIY1hmfK3Lcv1
TLSHT1B711023EA3DF9527ABD00A96568F327E428B403847520E5096CAD9DB124783A25F6F32
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