Debian Astro Radio Astronomy packages

• 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
• Santiago Vila

• 3.4.0-3 (trixie)
• 3.5.1-2 (sid)
• 3.0.0-2 (bullseye)
• 3.5.1-2 (forky)
• 3.1.0-2 (bookworm)

• 2 regular users
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• 98 total installations (of 284384 submissions)

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• Debian Astro Team
• Ole Streicher

• 3.7.1-1 (trixie)
• 3.8.0-5 (forky)
• 3.8.0-5 (sid)
• 3.3.0-4 (bullseye)
• 3.5.0-2 (bookworm)

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• 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
• Santiago Vila

• 5.0.1-3 (sid)
• 5.0.1-3 (forky)
• 4.2.0-1 (trixie)
• 2.0.0-5 (bullseye)

• 4 regular users
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• 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
• Santiago Vila

• 2.0.0-5 (bullseye)
• 4.2.0-1 (trixie)
• 5.0.1-3 (forky)
• 5.0.1-3 (sid)

• 5 regular users
• 16 recent
• 97 total installations (of 284384 submissions)

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• Debian Astro Team
• Ole Streicher

• 3.7.1-3 (sid)
• 3.3.1-1 (bullseye)
• 3.5.2-1 (bookworm)
• 3.7.1-2 (trixie)
• 3.7.1-3 (forky)

• 37 regular users
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• 226 total installations (of 284384 submissions)

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• 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

• 0.5.0-1 (bullseye)
• 0.6.0-3 (bookworm)
• 0.6.6-6 (forky)
• 0.6.6-2 (trixie)
• 0.6.6-6 (sid)
• 0.6.7 (upstream)

• 14 regular users
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• 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

• 3.7-1 (forky)
• 3.6-1 (trixie)
• 2.10.1-1 (bullseye)
• 3.1-3 (bookworm)
• 3.7-1 (sid)

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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)

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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)

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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.

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