Result for 104AD77E642E1BDD935C2322BC442AFD99D3F41C

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_step_combine.so
FileSize23960
MD54BAF4B1CE010DBDB08359649E2E2C5A5
SHA-1104AD77E642E1BDD935C2322BC442AFD99D3F41C
SHA-256F3BE399DF41AEB0BBC578AFF19EBB989EC0525F93A691557EBC14AFC53D01BD3
SSDEEP384:CJUI/bwgVZzj+gE0wYy7sfY7VFeB8z/lbT+czlUT:CJUI/bwsa/0wYyYwjeaR
TLSHT1FAB2B79AFF5A9A7BC4C232B8648F1371B3118788A31C53C3618C45A46F5536E4D7E58F
hashlookup:parent-total1
hashlookup:trust55

Network graph view

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
FileSize412076
MD508B3CE36677FB07D89A49E60A807357C
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-1EDDFA8E4D2940474F63B25AC9BDAB2C9340BD1C7
SHA-256F5CDE157AB1385847031F916C70B8A0015D5F3794F32164E289FACCEFEA462DA