Result for 14E5A6A516ADB47D82F19445995C5ACD64C43CA9

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_step_basic_calib.so
FileSize14136
MD5F897F0F68DD7BDCA044734D8C81B1E80
SHA-114E5A6A516ADB47D82F19445995C5ACD64C43CA9
SHA-25663C98E04F5D6F88FBBAC3D9F907C18D07781CD0AC95FCE79B7464C8C65914E69
SSDEEP384:f/DDNwz8ggTjNltLqWBPiS5QzG9fLkWwnIWU:3DJtfTRlJqWxVv
TLSHT1BD52968BB792DEB1C78121B4006B472EE6354831DA3FCF937D0C1198F4A96AD996335E
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
FileSize438120
MD5F14E612CDAC168854029D313E0FF1BC8
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-125C318905E702AE7B4F69DF645F83D37B0452B9E
SHA-256F63148016DA1AE247452781483A4BC1347D39621941BC5D9B51B2F5CE00EB9CD