Result for 1922051E027E9335EAF12D0B0F2F935CB249E437

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_apply_dist.la
FileSize1032
MD51A02C674AD3D36392A9C4A8E22A23682
SHA-11922051E027E9335EAF12D0B0F2F935CB249E437
SHA-256C2F84C5FE062440FC5113711A194899D5C9542C21B9CDEA01B4DC0E8288216D1
SSDEEP24:FpeSGsWJPbiNmmoxIY+Ahmfvi4rtvD2NGDe5/o0:FzGsWJPeNmmoxIY1hmfKARLco0
TLSHT18D11C33A934D5116EBD4158996CF313E428D883807AB2B54B3C7F5EF114F9161156E26
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
FileSize548756
MD57B774D5D5C690C1AD50BAFC43FDDB0C4
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
PackageVersion2.4.3+dfsg-1
SHA-1B6C87AC7CEF51846AD1962434E51181D948F75F9
SHA-2564BB11E9B6BA556172558877F98E9B23702C96254E0C6CD3DF42D3C2B65C795F7