Result for 1F9EC236B6791BB135EABAE2399981F1A825BABE

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.4.11/hawki_step_apply_dist.so
FileSize14488
MD5B3BF44343B8906845A417C9E02F4A5B4
SHA-11F9EC236B6791BB135EABAE2399981F1A825BABE
SHA-256195BE1F537C6A14B0CB3D240CD15396E33F36D3A2ACC1D476D1E238C5F15996C
SSDEEP384:EDgdZooXPVDggTjNltlbL2Gg5hYBK8z2R:2aZoo/FfTRlHbyGkYBf2
TLSHT15E52A54BBB91C971C3D221B45407072DA2714875E2BFDB837D4D2288EE957E8D9233AE
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
FileSize527876
MD51EDF8496263A6ADC7FA6A5315429C69F
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).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.4.11+dfsg-1
SHA-1B819EEA56280AD4ABCC44E5D419874F364EF861F
SHA-256591F4DC68AFEC363D198CBB54130A8FFCC76FF7F0F3FEE4034C8C6347C8CD4E0