Result for 04CD54578F18AA260ED3C6C30C8F888D856C2469

Query result

Key	Value
FileName	./usr/lib/x86_64-linux-gnu/hawki-1.8.18/libhawki.la
FileSize	956
MD5	769C21738EC5F17EFE1EB625E47E1B79
SHA-1	04CD54578F18AA260ED3C6C30C8F888D856C2469
SHA-256	8EBFD157F9A0FE889B52E6FDCF61861737ED0195FF98CE22ADD8F4843943E1CF
SSDEEP	12:o4fWgxhT/r5WFKiJLiORxI3a+AAmBB7Szf77ixCFlvT3RTZ/9IMCDwDqaAlH/HH0:jeShxWPimxIK+Ahmfvi4lvD2N0De5/0
TLSH	T1FC11E13BC39A463677E046554ADF302F834E443907570D1052CB99CB234381A31A6F72
hashlookup:parent-total	2
hashlookup:trust	60

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Parents (Total: 2)

The searched file hash is included in 2 parent files which include package known and seen by metalookup. A sample is included below:

Key	Value
FileSize	199012
MD5	B01C49B7C03387D9F4FEB6040374C806
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	1.8.18+dfsg-5
SHA-1	3471E1B68664943242AD6077ADE94A6DCD742EE6
SHA-256	318E3CDF027B1088E2BD10A59D696200CE37664D96E4CE2F5D0C6A0BDC7F1631

Key	Value
FileSize	198336
MD5	CA15E5417041E43053C886E1BDA5CD44
PackageDescription	ESO 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).
PackageMaintainer	Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageName	cpl-plugin-hawki
PackageSection	science
PackageVersion	1.8.18+dfsg-4
SHA-1	2F6AB05B3293B6E6D92D58EFCE8AE0437643F5A5
SHA-256	66C3B6431465CBAE37C289F7ECC5E28BFC824B5D82988FFBBC7C6CF67E5E805F