Result for 108911B0DA366900FE3A325E29DF98D45523FFBE

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_linearity_analyse.so
FileSize27872
MD5C670293A947DD7BFCECA9803FFD357CB
SHA-1108911B0DA366900FE3A325E29DF98D45523FFBE
SHA-256CCD98F338C004BCFD8CB013B052F075EBB90A211ABD1D92004387001EC5DDCFC
SSDEEP384:mDhQskHFyZASjV+M2rYoMUWk0wwruJZtXNHQ+WNPWS9h:mDhTkHt2gM2fMb7wdJnmRxWS9h
TLSHT112C2A86EFA1CFD27C5C6F339358A0761F3524A84A22047E3A56801886F4139E6D3E5DF
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