Result for 343EE6A68D3DC8A6B05F1D3B39E72D5C6D4CB38D

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-1.8.14/hawki_step_photom_2mass.so
FileSize22628
MD5E36DD2BC43B3C939A7B9BF81B2EDD38A
SHA-1343EE6A68D3DC8A6B05F1D3B39E72D5C6D4CB38D
SHA-256C46410D860A17E260549D1D2A897283C199D29863FF92F810055C2D1CDD05F20
SSDEEP384:OOl84NQiOeeRxIyvVMtzUgQuVZLW9y1DMymk45/7aewgK7Um/Ls6spoE+ia:OOl84iiOf3qz5QwLWE1DMyxY7aZY9h
TLSHT108A22ACFA54A3BA7C9C02F39589B0F5D22174AF092DC77034468C9346A959BE8732F4E
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
FileSize225126
MD5CF9FA4C7CE9F844C3D7E55B9BA5844E5
PackageDescriptionESO data reduction pipeline for HAWK-I 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
PackageVersion1.8.14+dfsg-2
SHA-1568F0F9D3C91E620D966913560B7CBEA3960D69E
SHA-256B4D26EE3EA7C0A8629B579288D4950615ED647084080BEA567F7948A39315B0B