Result for 1E10653160FC848BAC7AB5C8F00C839F32430AE1

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_step_basic_calib.so
FileSize15016
MD530ADB04A3D38D9CE5A59529295D5C1A6
SHA-11E10653160FC848BAC7AB5C8F00C839F32430AE1
SHA-2569FB618C77657391A13A6BBCBD246F78279BAAB861730D0A16A51CD905AB729DA
SSDEEP192:Ren8poDbCFeqzfqlofSFCsh+U5y1/nLcLwnIW2i6I0:kTD2FLKFCSy1ALwnIWiI0
TLSHT1D762D48BFA105DBEC5D1233480DB4A315978A8C4FF22C71B114C6179AA40398573FBAF
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
FileSize199012
MD5B01C49B7C03387D9F4FEB6040374C806
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-5
SHA-13471E1B68664943242AD6077ADE94A6DCD742EE6
SHA-256318E3CDF027B1088E2BD10A59D696200CE37664D96E4CE2F5D0C6A0BDC7F1631