Result for 270B64F5CD2A116C698EB920791CF34B2EAAEB2B

Query result

Key Value
FileName./usr/lib/powerpc-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_refine_offsets.so
FileSize67812
MD5D8640797BB7DB50622066F7B4090E3C8
SHA-1270B64F5CD2A116C698EB920791CF34B2EAAEB2B
SHA-256CE912BE827E3FCD06B0D7E683C3A07B34FF7E3ED303ADD00C8262DEF2C915A81
SSDEEP384:NXAl8MHHmqJg07mRM3OQRQe7T2kLgGxtgU4Uwx9WsDdrStP:NQl8MHgFQAkVuo
TLSHT14F638492A31F0C13C2B17B38155FA351832ECAC1E762466F114E1729399177C5ABAFEE
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
FileSize187838
MD5A024F16A962750A75766BD108C2F7C83
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
PackageVersion1.8.21+dfsg-1build1
SHA-120C6AEEBCCC03D080FE5001A90A75B22E3AC1CE9
SHA-256CBE18A9EE3DC715B90F92BCDC01F3CC3784AD46A1370F0A245A67339F4907F7E