Query result

Key	Value
FileName	./usr/lib/mipsel-linux-gnu/cpl/plugins/hawki-2.4.9/hawki_science_process.so
FileSize	90840
MD5	707BD164DB4623CF2B945DF7C0D5EF17
SHA-1	1D123E0B640D1C7E7AE49BFF76D1B43042BC97A4
SHA-256	C100191A44C996846E91010E956B35697DECD4057FD96E76C2A34372410F6EA6
SSDEEP	1536:ZKYVz6VVqi6qFIt62tlJFtpccWYQ83VS5/95/TnPpl/6ImKtQjmDN09ooUVxCXAZ:dIVVB6qFIt62tlJFtplWYQ83VS5/95/M
TLSH	T1CE93B252AF006E46D9D3CCB04D6DD5A1C6BF5D5E42ACBFA3BC5CC8847B0168CAD53898
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	451748
MD5	071B9F4695EF80D6D86B48ECB848BDB1
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	2.4.9+dfsg-1
SHA-1	2EFAE4DCB62A49CB19F7510008CFF9C14342BE11
SHA-256	ABAE21EFC2A432D5D37BD2D33604B5CE713A35277F7F34E80A7E278641E8009B