Result for 1C0EB15F8D3C81A2DC53E523532E63C6445E763D

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_util_gendist.la
FileSize1012
MD5E34BCB78058C3585EB92C5326D6B50F0
SHA-11C0EB15F8D3C81A2DC53E523532E63C6445E763D
SHA-2560DE7393FC43EA321435D577712B3A00E3939266549687B81B7FC6702FE6FF7A3
SSDEEP24:KXeSG1bWJYZiirr2xIY+Ahmfvi48d1vD2NGDe5/op:K9GVWJYAirr2xIY1hmfKvdpLcop
TLSHT10C11E27E835D6129A7D80AC5968E353F438D4038072D0E5852F6E5DB154F46D1197F26
hashlookup:parent-total2
hashlookup:trust60

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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
FileSize438120
MD5F14E612CDAC168854029D313E0FF1BC8
PackageDescriptionESO 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).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1build1
SHA-125C318905E702AE7B4F69DF645F83D37B0452B9E
SHA-256F63148016DA1AE247452781483A4BC1347D39621941BC5D9B51B2F5CE00EB9CD
Key Value
FileSize510596
MD5C3A8598255D089A56D7555D54E939763
PackageDescriptionESO 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).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1+b1
SHA-126EC7B533367155E98EE1068CED505920F9DD102
SHA-256AE2F773418C6EAFE9CB8230F334D27A87C21AD03F9D91B92A96859FA35E55D2F