Result for 2009CC5416DC898EB756B7222FDD71FC91FB4EEF

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_step_stats.so
FileSize68440
MD5D52FF975B0EBDF7F497CD831B15922E1
SHA-12009CC5416DC898EB756B7222FDD71FC91FB4EEF
SHA-256A0E85412BC021832E8CEC9198230F6B61D8F761A83FE183BA304B749A294DE8F
SSDEEP192:mr8i9wtCW+U2T7Ws76dft8cNTlPjlvOj5ZTkA3yQj88:ml9wEWM7ufZhg5KA328
TLSHT1466352A7B36E6B1ECF447535A1BF123523E26D0B172283039514A36A2ED5B7CCB3161B
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
FileSize547580
MD5B18CA767A1199AA5AF489CE17CD7BB65
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
PackageVersion2.4.3+dfsg-1
SHA-1F236FEA9C8FD567B3682BBF6658FCD7300D6B0E0
SHA-256F686E8D97B34E3D32A5A43F84F58708D1760617E24A4B37F15023F1F5FB5E51F