Result for 1B25D6142D752B692DA646A4D7343E1F49FD2B51

Query result

Key Value
FileName./usr/lib/mips-linux-gnu/cpl/plugins/hawki-1.8.21/hawki_step_photom_2mass.so
FileSize23096
MD55FB40163305B1495E08DA3C184E45BC1
SHA-11B25D6142D752B692DA646A4D7343E1F49FD2B51
SHA-2561D07D98943EC81EFEF649DA64C3607B372A2F7626A0B51A07D0BDC075F45DAB8
SSDEEP384:6Qk2Y3Ol8fMwrufnZDOLKfM1WkSMwh8dq7SS+SfFfGF9BXmNjlCM:6Qk2Y3Ol8fMwrg5UB/dq7FGF9J4N
TLSHT15CA2B55F33649D0DF0A2D3B8F4A7C6E51560556C29C19AB3C4BCF0422ACCA1FA53BD6A
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
FileSize226012
MD54C289725D3042772C3CC4229546F32DC
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
PackageVersion1.8.21+dfsg-1
SHA-1889A99B4EFD1D9875279122129BC03E6D652C846
SHA-2563E3320066BBF6E79776FAB1ECD889581BBED37D5A340ABF0247820338B9C6E8C