Result for 0EBF7C9C6B7A6A4D1FC85B7F95B8C4B0E42132F3

Query result

Key Value
FileName./usr/lib/mips-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_refine_offsets.so
FileSize19008
MD5393D2B312C55294E9E3B4ADD5385BD5C
SHA-10EBF7C9C6B7A6A4D1FC85B7F95B8C4B0E42132F3
SHA-256980DBB08B829CEEDA36070882901A92BFA0C04A2528FD67ECD9A7C81439E9CDB
SSDEEP192:/6vNAPV9ZkSgpchpfYto8pDnXAl3wlLlylHnlrADMXqBedGUWSIYM/2dNl2Fx27K:i1A9HGNXAl3wrIrkRBNsc202yE/EDJo8
TLSHT12D82A54F17259F4EF0E2C3BCA857C7D151B8486266CD0A63C83CB1516E88B0DA97FE66
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
FileSize226012
MD54C289725D3042772C3CC4229546F32DC
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
PackageVersion1.8.21+dfsg-1
SHA-1889A99B4EFD1D9875279122129BC03E6D652C846
SHA-2563E3320066BBF6E79776FAB1ECD889581BBED37D5A340ABF0247820338B9C6E8C