Result for 2F13BD1FB9F2C9E3FB0D9C99BACB5A8022773330

Query result

Key Value
FileName./usr/lib/powerpc64le-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_photom_2mass.la
FileSize1052
MD5A73F1FB57135FD0C9A3E340D0407D7B7
SHA-12F13BD1FB9F2C9E3FB0D9C99BACB5A8022773330
SHA-256DA2E67EBFD42D6F529D50AE5C774A194451F10F1AB3235E4D1F320B6B484911E
SSDEEP24:ueSGWWJNmifRxIY+Ahmfvi4qvD2NGDe5/B9xn:mGWWJNZxIY1hmfKPLcPx
TLSHT15B11423B839A1529AFE409466E8F747F43898539037D2E1452CBC4EF124B42932B6E22
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
FileSize224692
MD5D1343C262A1A7E0BD8BD4569E23F068D
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
PackageVersion1.8.21+dfsg-1
SHA-15671A6932A008A7BDE978A313EC947BFE2999B20
SHA-256136A0A4E926B114E41A51F5D4B1915255A9E2B8943770353493F216FBD564D4E
Key Value
FileSize190308
MD54A9C354B9047366270BE90C85A9082F1
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
PackageVersion1.8.21+dfsg-1build1
SHA-1255B34E4F87A4AB7107B747E7A67F6995239722E
SHA-256BB9CA8E6CCCE01596EB08FC791C6ECDF3554D3E2D18DC55330F7EDA7CAC17BBF