Searching for codes credited to 'Bell, M. E.'
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[ascl:1303.022]
ionFR: Ionospheric Faraday rotation
Sotomayor-Beltran, C.;
Sobey, C.;
Hessels, J. W. T.;
de Bruyn, G.;
Noutsos, A.;
Alexov, A.;
Anderson, J.;
Asgekar, A.;
Avruch, I. M.;
Beck, R.;
Bell, M. E.;
Bell, M. R.;
Bentum, M. J.;
Bernardi, G.;
Best, P.;
Birzan, L.;
Bonafede, A.;
Breitling, F.;
Broderick, J.;
Brouw, W. N.;
Brueggen, M.;
Ciardi, B.;
de Gasperin, F.;
Dettmar, R.-J.;
van Duin, A.;
Duscha, S.;
Eisloeffel, J.;
Falcke, H.;
Fallows, R. A.;
Fender, R.;
Ferrari, C.;
Frieswijk, W.;
Garrett, M. A.;
Griessmeier, J.;
Grit, T.;
Gunst, A. W.;
Hassall, T. E.;
Heald, G.;
Hoeft, M.;
Horneffer, A.;
Iacobelli, M.;
Juette, E.;
Karastergiou, A.;
Keane, E.;
Kohler, J.;
Kramer, M.;
Kondratiev, V. I.;
Koopmans, L. V. E.;
Kuniyoshi, M.;
Kuper, G.;
van Leeuwen, J.;
Maat, P.;
Macario, G.;
Markoff, S.;
McKean, J. P.;
Mulcahy, D. D.;
Munk, H.;
Orru, E.;
Paas, H.;
Pandey-Pommier, M.;
Pilia, M.;
Pizzo, R.;
Polatidis, A. G.;
Reich, W.;
Roettgering, H.;
Serylak, M.;
Sluman, J.;
Stappers, B. W.;
Tagger, M.;
Tang, Y.;
Tasse, C.;
ter Veen, S.;
Vermeulen, R.;
van Weeren, R. J.;
Wijers, R. A. M. J.;
Wijnholds, S. J.;
Wise, M. W.;
Wucknitz, O.;
Yatawatta, S.;
Zarka, P.
ionFR calculates the amount of ionospheric Faraday rotation for a specific epoch, geographic location, and line-of-sight. The code uses a number of publicly available, GPS-derived total electron content maps and the most recent release of the International Geomagnetic Reference Field. ionFR can be used for the calibration of radio polarimetric observations; its accuracy had been demonstrated using LOFAR pulsar observations.
[ascl:1408.023]
WSClean: Widefield interferometric imager
Offringa, A. R.;
McKinley, B.;
Hurley-Walker, N.;
Briggs, F. H.;
Wayth, R. B.;
Kaplan, D. L.;
Bell, M. E.;
Feng, L.;
Neben, A. R.;
Hughes, J. D.;
Rhee, J.;
Murphy, T.;
Bhat, N. D. R.;
Bernardi, G.;
Bowman, J. D.;
Cappallo, R. J.;
Corey, B. E.;
Deshpande, A. A.;
Emrich, D.;
Ewall-Wice, A.;
Gaensler, B. M.;
Goeke, R.;
Greenhill, L. J.;
Hazelton, B. J.;
Hindson, L.;
Johnston-Hollitt, M.;
Jacobs, D. C.;
Kasper, J. C.;
Kratzenberg, E.;
Lenc, E.;
Lonsdale, C. J.;
Lynch, M. J.;
McWhirter, S. R.;
Mitchell, D. A.;
Morales, M. F.;
Morgan, E.;
Kudryavtseva, N.;
Oberoi, D.;
Ord, S. M.;
Pindor, B.;
Procopio, P.;
Prabu, T.;
Riding, J.;
Roshi, D. A.;
Shankar, N. Udaya;
Srivani, K. S.;
Subrahmanyan, R.;
Tingay, S. J.;
Waterson, M.;
Webster, R. L.;
Whitney, A. R.;
Williams, A.;
Williams, C. L.
WSClean (w-stacking clean) is a fast generic widefield imager. It uses the w-stacking algorithm and can make use of the w-snapshot algorithm. It supports full-sky imaging and proper beam correction for homogeneous dipole arrays such as the MWA. WSClean allows Hogbom and Cotton-Schwab cleaning, and can clean polarizations joinedly. All operations are performed on the CPU; it is not specialized for GPUs.