Result for 0C69E17E6D09EF29AF9C2CC04EDF091EB1FCF029

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_util_stdstars.so
FileSize9860
MD568A11150E0EFB8EFAF2AC13462AEC2DE
SHA-10C69E17E6D09EF29AF9C2CC04EDF091EB1FCF029
SHA-25684FCE6A53E7EAE6DB08A78B2DEB1C2DE7BB8465C1C2A26CFEC48BB0355E099E7
SSDEEP192:D8p/jJ4M04zX3Qgc2EwhHqgtUVSYtJXprTSUUEX6:0XHggTTkJBuUUl
TLSHT14912A80AFBC7D9B2E2D951B8914BD23EDA318404AA47C3A3755877DC5C22BC8CB1177A
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
FileSize221550
MD57CA8C8F751AC49CD58D14D76DA00B8B5
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-1BA8CEACF21DD0E05B10A5C496CD082AD9365547E
SHA-256949029E1EA39C0BBA2A85405157D2B6E9179DF9FAFA1E585C720E7DE40B0B7D9