Result for 116A365AABB7F35D1AD0EE34180A1DA7630C487A

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_step_photom_2mass.so
FileSize23688
MD5969313DC729651ADFF737C3556F93178
SHA-1116A365AABB7F35D1AD0EE34180A1DA7630C487A
SHA-256517C127EB8ADB6A40349655CF60B7951C24D6B05540951303FBE38B41A67312A
SSDEEP384:xgOl8A2ndYgkt9MPAYrLwMl3/eVgTpeL:xgOl8A2nmgk/CRrLwCeCTw
TLSHT136B20797E751CABCC8C4A730A4CF5426A2307814E73DA32B57C41B769E2231D972B79B
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