Query result

Key	Value
FileName	./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.8/hawki_science_process.so
FileSize	90840
MD5	E8E66E3D6A003C37AA8722B8F7E1ECA5
SHA-1	005EECBE7F1FF32E95B32EEA79E3788C2074F409
SHA-256	19B55C2AFDA7AB25D623BAAAD4FBB352EC70DEDF7FFADDA6E4036F63B7FD3A86
SSDEEP	1536:TDrOVzhXVKb/lzI562tlJFtppWIi83VS5/95/rOQjmYu09ooUVxCXRv//vnKTFb/:/yPXVw/lzI562tlJFtppWIi83VS5/95e
TLSH	T17F93A192AF046E47D8D3CCB04EADD461C6BF5D6E42ACBEA3BC5CC8947B0164CAD53858
hashlookup:parent-total	1
hashlookup:trust	55

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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
FileSize	451824
MD5	1F48F63051D9F44902CAF24A014F7EA7
PackageDescription	ESO 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).
PackageMaintainer	Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	2.4.8+dfsg-4
SHA-1	1F8850C8DF01377F7D9588E80BA2C9DB502D4044
SHA-256	0A8C64809D35D4085A35B94D11899977427986C005708D095B5B089F504E52EE