Result for 14F8052870F04C8386EC5B47491EC557EA1B6883

Query result

Key Value
FileName./usr/lib/i386-linux-gnu/hawki-2.4.3/libhawki.so.0.0.0
FileSize577724
MD5A7F76B944AB6A9B249408143FC97D241
SHA-114F8052870F04C8386EC5B47491EC557EA1B6883
SHA-2565B1486FCDD790C7D4326160A1A03A7D00439C6DDDF4AA8754D0D23B1CA9E7436
SSDEEP12288:YHApYu00v99gOhaCDPK2hEdkkzFRnp3W7bKWUWdRDtVA:YgpYk7gOwcKOEd/np3uuWU0J
TLSHT17BC40A5EE7838CE3F2D255B517535636CD248E09E037F2F29E8A72553435A883E2B263
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
FileSize548756
MD57B774D5D5C690C1AD50BAFC43FDDB0C4
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
PackageVersion2.4.3+dfsg-1
SHA-1B6C87AC7CEF51846AD1962434E51181D948F75F9
SHA-2564BB11E9B6BA556172558877F98E9B23702C96254E0C6CD3DF42D3C2B65C795F7