Result for 177595D5B9BF8CE1F862A44303ECD1075172E772

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_cal_dark.so
FileSize22780
MD5A1E7B9FA377F53E2799FCDB39897366C
SHA-1177595D5B9BF8CE1F862A44303ECD1075172E772
SHA-2566E30EDF9591229409B18DF10481BF5291CB41FB7734EB115105ECE43887037A6
SSDEEP384:B1VjbWggTjNltlCH8TgvTBVKIxW1UiPdyijL1c:B15bWfTRlHCcstYcW1UmQ
TLSHT1CAA2E583FEC7C5F0D6D32532410BAA2F8A74A512EE16C743FD4C2786E52271C8925B6E
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
FileSize196654
MD50A2841A209224E251882DC665A2EB149
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
PackageVersion1.8.14+dfsg-2
SHA-1B2471E6CD8501B5A1B43B2EC659031EB8B478ED9
SHA-256332FEEC118B1D561CAAF58D189027595FB6AF81FF18CF0C8BEF702BFC56BB89A