Result for 15356414D1E4F585A9A5875C39B6502867D753A7

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_dark_combine.so
FileSize28272
MD5E4013D43D9B2EFBEC2C12DDA7D458218
SHA-115356414D1E4F585A9A5875C39B6502867D753A7
SHA-2566016A6D6D1E0D099D463A40FCCC811343649A67867F907F3A97713AA171EF0DE
SSDEEP384:zsI3yUAvqI5yHeYnXaTJWHg/byBIFi0uzgrcT:z3uCIwL8JWHgzyhhErcT
TLSHT11BC285BEBE189937C893E23955CA1710F32246E8B2304BD37A5915182F41FDE893F69D
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
FileSize446980
MD516EFB69819EAF8E09B64CBD57CC67A9B
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
PackageVersion2.4.9+dfsg-1
SHA-1BAF855C0E5F8829D60769AF9482EFE8ED23EFB36
SHA-2560E43A15CEC1735CDE3AE4C7FF1A00C540392D2A763450F033F2AB8EAEB957702