Result for 1CAA066D48FAE57D067228B58749F06FA08D7E00

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_cal_flat.so
FileSize41120
MD587BDB42566DC53C6DEDB1411DEEB1479
SHA-11CAA066D48FAE57D067228B58749F06FA08D7E00
SHA-256D703BA35B4A7039D4BFE49887E82A67A098D817FE11570CCB0687302FDBCADEB
SSDEEP768:hub60GF9hO6c5DdkUU4BvaToKEv6EBjnqQaOErv:hu+0PNkUU4BSoKEyERn/Erv
TLSHT17303084FA5729675C1E0D734D9FF5302A8B47880FB3597AB268862715A0237C432EB6F
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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