Result for 063C5991B87533BBEB9DB3A9814BD566A0AAA833

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.18/hawki_step_refine_offsets.so
FileSize19704
MD5009C18A1D70471C3FB121383E8F2756B
SHA-1063C5991B87533BBEB9DB3A9814BD566A0AAA833
SHA-2560A2CF1C20B2EA0037C0433B798912822C67011BADE49C96D8EFB7BCD9357BA26
SSDEEP192:RFu68pDnXAlPbd4aE3k2hwbJPtXieX6N8x2JR2X4rxQ3i:/wXAlTd2mJVytNLJRt
TLSHT158920ACFEA165776C0E89334A0CB19502870B895F724971B198892707E07B1C5FAFBAF
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize199012
MD5B01C49B7C03387D9F4FEB6040374C806
PackageDescriptionESO data reduction pipeline for HAWK-I 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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.18+dfsg-5
SHA-13471E1B68664943242AD6077ADE94A6DCD742EE6
SHA-256318E3CDF027B1088E2BD10A59D696200CE37664D96E4CE2F5D0C6A0BDC7F1631