aoflagger 3.1.0-2build3 source package in Ubuntu

Changelog

aoflagger (3.1.0-2build3) jammy; urgency=medium

  * No-change rebuild with Python 3.10 as default version

 -- Graham Inggs <email address hidden>  Sat, 15 Jan 2022 08:33:12 +0000

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Uploaded by:
Graham Inggs
Uploaded to:
Jammy
Original maintainer:
Ubuntu Developers
Architectures:
any
Section:
misc
Urgency:
Medium Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Jammy release universe misc

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File Size SHA-256 Checksum
aoflagger_3.1.0.orig.tar.gz 978.3 KiB 86a83cd8b90bde24d8c9533cbccdfddc9d3b2ed9cc74f082456bc1a975883e60
aoflagger_3.1.0-2build3.debian.tar.xz 9.3 KiB c252f4fe53cdc43a610fda237ea6f245638f1bf72149900b1ab9c4da5fe38c9c
aoflagger_3.1.0-2build3.dsc 2.5 KiB 47aa269bd7336688cc68931e06e3fd1ffdb5bc484f3f82516a7ec9276d38a385

Available diffs

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Binary packages built by this source

aoflagger: Find RFI in radio astronomical observations

 The AOFlagger is a tool that can find and remove radio-frequency interference
 (RFI) in radio astronomical observations. The code has been highly optimized
 for speed and accuracy. It is used by default for the LOFAR radio telescope
 and thus is in productional stage. The software can run in a fully automated
 way, but a graphical interface is provided to analyse results and tweak the
 strategy. The preferred input file format is the Casa Measurement Set (MS)
 format.
 .
 Besides the flagger, the software consists of tools to efficiently visualize
 data in different ways, such as plotting time-frequency diagrams and power
 spectra. It provides the programs aoflagger, rfigui, aoqplot, aoquality and
 more.

aoflagger-dbgsym: No summary available for aoflagger-dbgsym in ubuntu kinetic.

No description available for aoflagger-dbgsym in ubuntu kinetic.

aoflagger-dev: No summary available for aoflagger-dev in ubuntu kinetic.

No description available for aoflagger-dev in ubuntu kinetic.

libaoflagger0: Find RFI in radio astronomical observations (shared lib)

 The AOFlagger is a tool that can find and remove radio-frequency interference
 (RFI) in radio astronomical observations. The code has been highly optimized
 for speed and accuracy. It is used by default for the LOFAR radio telescope
 and thus is in productional stage. The software can run in a fully automated
 way, but a graphical interface is provided to analyse results and tweak the
 strategy. The preferred input file format is the Casa Measurement Set (MS)
 format.
 .
 This package contains the shared library.

libaoflagger0-dbgsym: debug symbols for libaoflagger0