Query result

Key	Value
FileName	./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.2.0/hawki_science_postprocess.so
FileSize	44052
MD5	B30BB6E693AA18D176AAE16C82A28176
SHA-1	0C4E2C173C6AFACC0566D0A1FCD0233A5AF3A062
SHA-256	D81996F8FB88551AC53166398DEC0D18D95BE836FCE43BAD6CFE1C1CCD147CBD
SSDEEP	768:vsm7lCv6pq2w8IPO7Y3LEKyqAqYJc3DKFYJGYyVjYffPqyyyyyyyyyyyyyyyyyy2:Em7lCvUw8lk3LE3qYJcTKFYJGYE
TLSH	T1971308C2E9A55F9BC2C06735367E4769332386B4D3EF7757882992286A0320E4D25F9C
hashlookup:parent-total	1
hashlookup:trust	55

Network graph view

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	442062
MD5	E779873E6D359675CEDBC17AC57E9320
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	2.2.0+dfsg-1+b1
SHA-1	3C5CD869CACE89525DD780CA8081A8C6802AEDE3
SHA-256	EB202A58AA0E86581745FF06F55E29A9F37826AF733B571458392DCD61AAD19D