Result for 0CF819126B2F597E0DC04C9D5862C70ECA956867

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_sci_jitter.so
FileSize45328
MD5F6AACA863AD32887FF6A82B282D51CD3
SHA-10CF819126B2F597E0DC04C9D5862C70ECA956867
SHA-2561E90514D3C15705BABF7D327AE359CC94EF8D3FC2D1EAA3E15B7969709103E8B
SSDEEP768:scFxuw7597XDWUtMbE4QxaLicnt9UKMbS9uIqP:scewTzWoMbE4nLiigKMbB3
TLSHT19D13088BB6A14BB2C5D4A730A9DF24455970B892F6389B1F154843746D02B6CE33FF2B
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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