Searching for codes credited to 'Kaplan, D. L.'
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[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.
[ascl:2011.017]
RRATtrap: Rotating Radio Transient identifier
Karako-Argaman, C.;
Kaspi, V. M.;
Lynch, R. S.;
Hessels, J. W. T.;
Kondratiev, V. I.;
McLaughlin, M. A.;
Ransom, S. M.;
Archibald, A. M.;
Boyles, J.;
Jenet, F. A.;
Kaplan, D. L.;
Levin, L.;
Lorimer, D. R.;
Madsen, E. C.;
Roberts, M. S. E.;
Siemens, X.;
Stairs, I. H.;
Stovall, K.;
Swiggum, J. K.;
van Leeuwen, J.
RRATtrap is a single-pulse sifting algorithm to identify Rotating Radio Transients (RRATs) and transients using output from the PRESTO (ascl:1107.017) routine single_pulse_search.py. It can be integrated into pulsar survey data analysis pipelines and, in addition to finding RRATs, it can also identify Fast Radio Bursts.