Result for 09B716D6E23840B4233BF127CF49A91067CF813B

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.9/hawki_step_combine.so
FileSize23268
MD5CABDE55C7B6E402DF52EAAE432B893AB
SHA-109B716D6E23840B4233BF127CF49A91067CF813B
SHA-256747331FE7E46B2CAE34E0709E1A76DF3B17B3A4F2778DB73FEFA86D8AFC7F2DE
SSDEEP384:RSTI/tnIPp22V7lkGYaieznGEiNrAVU3LfU6kp4xZSDGmbT+czlU:RSTI/tIw2VpkGhiezn/w0VU3DUU1m
TLSHT16CA2D7CFB5137A67D0C02E35350F4B0A62238DA9D29C6716856C4D202D077FD9EA6A6E
hashlookup:parent-total1
hashlookup:trust55

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Parents (Total: 1)

The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize453352
MD55CFC0CB5C37652E14DA39B16073327E6
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
PackageVersion2.4.9+dfsg-1
SHA-109AD28C108CC2A32C4F9E9E6E17CB27DA90FFD5E
SHA-2567A78D83C1E6E73EB9D53CA7D68B3C5EB49076AFE08652C402C0E2888B970DE64