Result for 11AEB6A843F04639EF66EE5757CB6B2DF509422E

Query result

Key Value
FileNamehawki_cal_distortion.so
FileSize31172
MD5B7A0356A42D26B2454B8245129C2EC8A
RDS:package_id182052
SHA-111AEB6A843F04639EF66EE5757CB6B2DF509422E
SHA-2569E05866BC37691ACDA7D578F0801CC5EE39A8B6D737C5359A2BCD234A81A5627
SSDEEP768:3xAliABfTRlHCcQMji7pEfXNqmYmqwKn8hHU:BZAtXQmfXNqTVwz0
TLSHT1B3E2C5CFE5E2C8B1FAC221F51C57466585309550E72BC3D2AB083A85562329DFAB373B
insert-timestamp1679423153.3206565
sourceRDS.db
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
FileName13697
FileSize222964
MD5974C59296FB3D0C20D19308DD77F09D1
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
RDS:package_id182052
SHA-14E0EAFAA7F8F95F0090AB88C11D17F77A12BCCFE
SHA-256266882D5AE449DE6BE617369A30F14C4281B4D1A395A3C0695B24BA38DAC0ADE
insert-timestamp1679408379.314181
sourceRDS.db