Debian Astro Radio Astronomy packages

AOFlagger er et værktøj, som kan finde og fjerne interferens for radiofrekvenser (RFI) i radioastronomiske observationer. Koden er blevet optimeret for hastighed og præcision. Bruges som standard for LOFAR-radioteleskopet og er derfor i produktion. Programmet kan afvikles på en fuld automatiseret måde, men en grafisk grænseflade tilbydes til at analysere resultater og finjustere strategien. Det foretrukne filformat er formatet Casa Measurement Set (MS).

Denne pakke indeholder teksthovedfilen til at kompilere egne programmer mod biblioteket.

• A. R. Offringa, A. G. de Bruyn, M. Biehl, S. Zaroubi, G. Bernardi and V. N. Pandey: Post-correlation radio frequency interference classification methods. Monthly Notices of the Royal Astronomical Society 405:155 - 167 (2010) (eprint)

• Debian Astro Team
• Ole Streicher

• 2.13.0-1 (buster)
• 2.9.0-1 (stretch)
• 3.4.0-2 (sid)
• 3.4.0-2 (trixie)
• 3.1.0-2 (bookworm)
• 3.0.0-2 (bullseye)

• 3 recent
• 75 total installations (of 236226 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

• Upload Screenshot
• Create tags

Pakken casacore indeholder basisbibliotekerne for den gamle pakke AIPS++/CASA (Common Astronomy Software Applications). Denne opdeling blev lavet for at få en bedre separation af basisbibliotekerne og programmer.

Denne pakke indeholder filerne for programudvikling.

• Debian Astro Team
• Benjamin Drung

• 3.0.0-4 (buster)
• 3.5.0-2 (bookworm)
• 3.5.0-4 (trixie)
• 3.3.0-4 (bullseye)
• 2.2.0-2 (stretch)
• 3.5.0-4.1 (sid)

• 3 recent
• 83 total installations (of 236226 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

• Upload Screenshot
• Create tags

PURIFY er en samling af rutiner skrevet i C, der implementerer forskellige værktøjer for radiointerferometrisk billeddannelse inklusive filhåndtering (for både visibilities- og fits-filer), implementering af måleoperatøren og opsætning af forskellige optimeringsproblemer brugt for billeddekonvolution. Koden kalder den generiske pakke Sparse OPTimization (SOPT) for at løse billedoptimeringsproblemer.

Denne pakke indeholder udviklingsfilerne.

• Luke Pratley, Jason D. McEwen, Mayeul d'Avezac, Rafael E. Carrillo, Alexandru Onose and Yves Wiaux: Robust sparse image reconstruction of radio interferometric observations with PURIFY. Mon. Not. Roy. Astron. Soc., submitted (2016) (eprint)

• Debian Astro Team
• Nilesh Patra

• 2.0.0-5 (bullseye)
• 2.0.0-1 (stretch)
• 2.0.0-6 (sid)
• 2.0.0-4 (buster)
• 4.0.0-alpha (upstream)

• 61 total installations (of 236226 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

• Upload Screenshot
• Create tags

PURIFY er en samling af rutiner skrevet i C, der implementerer forskellige værktøjer for radiointerferometrisk billeddannelse inklusive filhåndtering (for både visibilities- og fits-filer), implementering af måleoperatøren og opsætning af forskellige optimeringsproblemer brugt for billeddekonvolution. Koden kalder den generiske pakke Sparse OPTimization (SOPT) for at løse billedoptimeringsproblemer.

• Luke Pratley, Jason D. McEwen, Mayeul d'Avezac, Rafael E. Carrillo, Alexandru Onose and Yves Wiaux: Robust sparse image reconstruction of radio interferometric observations with PURIFY. Mon. Not. Roy. Astron. Soc., submitted (2016) (eprint)

• Debian Astro Team
• Nilesh Patra

• 2.0.0-1 (stretch)
• 2.0.0-4 (buster)
• 2.0.0-5 (bullseye)
• 2.0.0-6 (sid)
• 4.0.0-alpha (upstream)

• 1 regular users
• 62 total installations (of 236226 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

• Upload Screenshot
• Create tags

Pakken casacore indeholder de grundlæggende biblioteker for den gamle AIPS++/CASA-pakke. Denne opdeling blev lavet for at få en bedre adskillelse af de grundlæggende biblioteker og programmer. CASA er nu bygget oven på casacore.

Dette er Pythonomslaget omkring biblioteket.

• Debian Astro Team
• Ole Streicher

• 3.3.1-1 (bullseye)
• 3.5.2-1 (bookworm)
• 3.0.0-1 (buster)
• 2.1.2-3 (stretch)
• 3.5.2-1 (sid)
• 3.5.2-1 (trixie)

• 28 regular users
• 5 recent
• 213 total installations (of 236226 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

• Upload Screenshot
• Create tags

Pakken spectral-cube tilbyder en nem måde at læse, manipulere, analysere og skrive datakuber med to positionsdimensioner og en spektraldimension, valgfrit med Stokes parametre. Forsøger at være en alsidig datacontainer til at bygge tilpassede analyserutiner.

• A. Ginsburg, T. Robitaille, C. Beaumont, E. Rosolowsky, A. Leroy, C. Brogan, T. Hunter, P. Teuben and D. Brisbin: Radio Astronomy Tools in Python: Spectral-cube, pvextractor, and more. Revolution in Astronomy with ALMA: The Third Year :363 (2015) (eprint)

• Debian Astronomy Team
• Ole Streicher

• 0.6.0-3 (bookworm)
• 0.6.5-3 (sid)
• 0.6.5-3 (trixie)
• 0.5.0-1 (bullseye)
• 0.4.3-2 (buster)
• 0.4.0-2 (stretch)

• 4 regular users
• 3 recent
• 153 total installations (of 236226 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

• Upload Screenshot
• Create tags

WSClean (w-stacking clean) er en hurtig generisk widefield imager. Programmet bruger algoritmen w-stacking og kan bruge algoritmen w- snapshot. Fra og med februar 2014 er den 2-12 gange hurtigere end CASA's w- projektion, afhængig af tabelkonfigurationen. Programmet understøtter full- sky imaging og korrekt beam-korrektion for homogene dipole tabeller såsom MWA'en.

WSClean tillader Hogbom og Cotton-Schwab-oprydning, og kan rydde op i polarisationer sammen. Alle operationer udføres på cpu'en (programmet er ikke specialiseret for GPU'er).

Denne pakke indeholder det statiske bibliotek og teksthovedfiler til at kompilere egne programmer mod biblioteket.

• A. R. Offringa, B. McKinley, N. Hurley-Walker, F. H. Briggs, R. B. Wayth, D. L. Kaplan, M. E. Bell, L. Feng, A. R. Neben, J. D. Hughes, J. Rhee, T. Murphy, N. D. R. Bhat, G. Bernardi, J. D. Bowman, R. J. Cappallo, B. E. Corey, A. A. Deshpande, D. Emrich, A. Ewall-Wice, B. M. Gaensler, R. Goeke, L. J. Greenhill, B. J. Hazelton, L. Hindson, M. Johnston-Hollitt, D. C. Jacobs, J. C. Kasper, E. Kratzenberg, E. Lenc, C. J. Lonsdale, M. J. Lynch, S. R. McWhirter, D. A. Mitchell, M. F. Morales, E. Morgan, N. Kudryavtseva, D. Oberoi, S. M. Ord, B. Pindor, P. Procopio, T. Prabu, J. Riding, D. A. Roshi, N. U. Shankar, K. S. Srivani, R. Subrahmanyan, S. J. Tingay, M. Waterson, R. L. Webster, A. R. Whitney, A. Williams and C. L. Williams: WSCLEAN: an implementation of a fast, generic wide-field imager for radio astronomy. Monthly Notices of the Royal Astronomical Society 444:606 - 619 (2014) (eprint)

• Debian Astro Team
• Ole Streicher

• 3.4-1 (trixie)
• 2.10.1-1 (bullseye)
• 3.1-3 (bookworm)
• 2.2.1-1 (stretch)
• 2.6-1 (buster)
• 3.4-1 (sid)

• 3 recent
• 81 total installations (of 236226 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

• Upload Screenshot
• Create tags

Aperture synthesis or synthesis imaging is a type of interferometry that mixes signals from a collection of telescopes to produce images having the same angular resolution as an instrument the size of the entire collection. At each separation and orientation, the lobe-pattern of the interferometer produces an output which is one component of the Fourier transform of the spatial distribution of the brightness of the observed object. The image (or "map") of the source is produced from these measurements. Astronomical interferometers are commonly used for high-resolution optical, infrared, submillimetre and radio astronomy observations.

This package contains the header files for development.

• Debian Astro Team
• Gijs Molenaar

• 0.1-1 (VCS)

• Announcement
• Git

• Home page

The OSKAR package consists of a number of open source libraries and applications for the simulation of astronomical radio interferometers. OSKAR has been designed primarily to produce simulated data from large aperture arrays, such as those envisaged for the SKA.

• F. Dulwich, B. J. Mort, S. Salvini, K. Zarb Adami and M. E. Jones: OSKAR: Simulating Digital Beamforming for the SKA Aperture Array. Wide Field Astronomy & Technology for the Square Kilometre Array :31 (2009) (eprint)

• Debian Astro Team
• Gijs Molenaar

• 2.6.1-1 (VCS)

• Announcement
• Git

• Home page

SAGECal is a very fast, memory efficient and GPU accelerated radio interferometric calibration program. It can handle all source models including points, Gaussians and Shapelets. It can calibrate along hundreds of directions without running out of memory in almost real time. Intel Xeon Phi acceleration is also available. Distributed calibration using MPI and consensus optimization is enabled. Also tools to build/restore sky models are included.

• Announcement
• Vcs

• Home page