Result for 17D4A7AED1ADAA9D0787E3E2524E842C9B94796C

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.11/hawki_step_combine.so
FileSize68324
MD535B8B062D980A9559A37DCED074FCADB
SHA-117D4A7AED1ADAA9D0787E3E2524E842C9B94796C
SHA-2567BD7C6167BC1F8EB6D9324812FF8E321B019989DD3CEC5905733AEE786EBE5FC
SSDEEP384:xSvI/tnQc7l/vmxZ3ej9zAuR01hsWDB7VLfKkp4xkSdisbT+czlULf:xSvI/tdp2xZ3iRRXW17VDZ9s6f
TLSHT1B663D6DF75726BA7C0C06FB4640B0B1DB32785A4879967128A1842312F826FD5F37B9E
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
FileSize460432
MD5C4C5EBB37D7DBB8298549F3C6954D382
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-1CD3572D24E59B9C5CC2677F15ACDA24FFDA85C4C
SHA-2564ACCFB4EC42FBCD04415B3421FF1F11B47DE7CE1669F475BEC1727F12E938654