Result for 109AF62E6E8FEEFCE08FF8DDAD7D62DB66B08D57

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_cal_distortion.so
FileSize28088
MD5774900EE0B242C957832C02DD8DF3ADA
SHA-1109AF62E6E8FEEFCE08FF8DDAD7D62DB66B08D57
SHA-256A91EA1B59CB65D3E7C50CD9CBD665DAC99DA42F7F1804390C52E8B81938D2339
SSDEEP384:208XidS2DJQbW/uX6DSXAekJEf+6qEDe5hsc:208XO5du5iekWWI
TLSHT108C209AFA5605A7AC4D593B098CB19215DB07950FB34A70E560851B83F09BBCE33F72B
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
FileSize407134
MD58BB75CFCA14D06B369847DA5AD3C0659
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument 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
PackageVersion2.2.0+dfsg-1build1
SHA-157E12B5F92879BB2A2B01FC61AE6BF5307FC2945
SHA-2560A0320B5C8F5B44A2C6CBD2E98BE1B3BEC71DBF24EF43CE8BC2912388B5663DD