Result for 0305CB89FD898652F02905DAD899687398A2B23D

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_compute_bkg.so
FileSize23856
MD5BDD6F8C7FA34E39A3B9D1BE10C82DB94
SHA-10305CB89FD898652F02905DAD899687398A2B23D
SHA-25677C91276ADB299020E174662CB421A9C74F6BF73FF2B5A07F8DB401C40F83A1F
SSDEEP384:2Sna8UVwrbBuAyG/j5S9dZrRkDJZDt9TQrLOGSmdKUx0y:XnRh1uAyWj89PRAQL
TLSHT1D7B2F969FE49992FCCD2F2B9618F0734B3210C0CA3499793748C46A52F0C2BE9D7759A
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
FileSize166042
MD5B97749A724F73C32C3325C17663564D8
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-11A54E42B7554DE056107B4700225D916C9932974
SHA-2560E51D833B4411CD82D6A2A5FE156078517284A85462E8AC7D767EF137DF6136F