Result for 012B340F061CBD9A474ACB17295637D2B2F3A0D7

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabihf/cpl/plugins/hawki-2.2.0/hawki_cal_zpoint.la
FileSize1005
MD5858AE6603F552A2C8F7ABBC9E4E0E519
SHA-1012B340F061CBD9A474ACB17295637D2B2F3A0D7
SHA-25679448570D1B6C94DFF4575732B48C69B895925E95C4B90DBA1E7518DB179015E
SSDEEP24:4eSG1bWJ+izxIY+Ahmfvi4IvD2NGDe5/AjY:UGVWJ7zxIY1hmfK3LcAM
TLSHT11511023EE3DF9527ABD00997568F327E528F403807520E5092CAD5DB124743925F6F23
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
FileSize426848
MD5C8FC8B61CFE578FB387193CC0948C4CE
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-10D7A9C3BDB5386D1AD3C03E278B8A26A53117B63
SHA-256E99CF0D36C035AAC0C944D8858B13809B9E0F719118FEA0D5165C368314DEA9E
Key Value
FileSize353598
MD5A1BD40963DB2A77A0D7730FE85D0AF94
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-1EB736B139332F6B26DE6CFF7CB6FC31819963E2A
SHA-25697C93587330F9AE975DB4E10FD12ADD6E9FA3078083991808F019B208598BCBD