Result for 0A4FC4655289E1D73562D5AAB2FFFB315B68B13E

Query result

Key Value
FileName./usr/lib/arm-linux-gnueabi/cpl/plugins/hawki-2.4.8/hawki_step_stats.so
FileSize10548
MD5D0A5956E76FD074D31F252F91951054E
SHA-10A4FC4655289E1D73562D5AAB2FFFB315B68B13E
SHA-256F93409D2D0B383F81187A44571EB415804C491D4D9C39ADEC2DFFE0CB8D94B45
SSDEEP192:od8q+NGZ2H9QkNXiLxPCaxmxM4lLfPYPjlPFKtF3yQ:of+NGZ2HfNXLlLfPkh83
TLSHT1FB22638DB2A74E63CDD02539B15B0E2A2B9189965357AF13550C33A02D2B6784D3AF2A
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
FileSize454368
MD560DE75C96E5EEC0B0CB809D3B38C05AD
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
PackageVersion2.4.8+dfsg-4
SHA-12362C669BEDA660467F4EAF89E0BD6020E351A71
SHA-256A6CE560A5A7EC6D78F19A88181F56DD7D73263A6DDB72A6C829DD442A9F575A1