Result for 03A1EA1E34E06AE1AB2BBCCE9BA1299AA422F01E

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_stitch.la
FileSize1012
MD56E46FD614A4FBA1E54270AEF2DCB0A8B
SHA-103A1EA1E34E06AE1AB2BBCCE9BA1299AA422F01E
SHA-2565AF8BA569EFBC23BC2822039AE059EBDC5A34E452E102A400949BABB52A1D9EB
SSDEEP24:HeSGWWJvikxIY+Ahmfvi4tvD2NGDe5/vxn:tGWWJKkxIY1hmfKaLcvx
TLSHT10911323A939A5135AFD00A895B8F723E4789487C07710F5062FB85DB128B81A2556E33
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
FileSize203830
MD50217B24BC288D83D67B33CC086B6DC72
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-1A3D2F47DDC44170E6E18F65F24ECF6BC5365A200
SHA-2568BAD397247F133240BFF3538BA243E921F9D81B6F302F0F295AE0F28FE15DF22
Key Value
FileSize166042
MD5B97749A724F73C32C3325C17663564D8
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-11A54E42B7554DE056107B4700225D916C9932974
SHA-2560E51D833B4411CD82D6A2A5FE156078517284A85462E8AC7D767EF137DF6136F