Result for 2A9ACE6E904373291505CE8A3486507B45FADD02

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_step_detect_obj.so
FileSize23928
MD5B06FD03F2C356E6AC587154B22F56335
SHA-12A9ACE6E904373291505CE8A3486507B45FADD02
SHA-2563C76C75C6A89F1E116ADD7FF0F6FD9F972B4CBA9CBDEC7B7E74B77491ED02E4A
SSDEEP384:fdoxJBoSGyRv8nxmj7rxXvCtpUCrGkFMMgDKxI0:WxJBoJ/n8XvUpr0
TLSHT178B2098FE1116BB6C8D8B73098DB16252630F554FA34D63B309816B45A41B9C8B3F7AF
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
FileSize198336
MD5CA15E5417041E43053C886E1BDA5CD44
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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.18+dfsg-4
SHA-12F6AB05B3293B6E6D92D58EFCE8AE0437643F5A5
SHA-25666C3B6431465CBAE37C289F7ECC5E28BFC824B5D82988FFBBC7C6CF67E5E805F