Astronomical wide-field imaging of interferometric radio data is computationally expensive, especially for the large data volumes created by modern non-coplanar many-element arrays. We present a new wide-field interferometric imager that uses the w-stacking algorithm and can make use of the w-snapshot algorithm.
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- Offringa, A. R. (Author)
- McKinley, B. (Author)
- Hurley-Walker, N. (Author)
- Briggs, F. H. (Author)
- Wayth, R. B. (Author)
- Kaplan, D. L. (Author)
- Bell, M. E. (Author)
- Feng, L. (Author)
- Neben, A. R. (Author)
- Hughes, J. D. (Author)
- Rhee, J. (Author)
- Murphy, T. (Author)
- Bhat, N. D. R. (Author)
- Bernardi, G. (Author)
- Bowman, Judd (Author)
- Cappallo, R. J. (Author)
- Corey, B. E. (Author)
- Deshpande, A. A. (Author)
- Emrich, D. (Author)
- Ewall-Wice, A. (Author)
- Gaensler, B. M. (Author)
- Goeke, R. (Author)
- Greenhill, L. J. (Author)
- Hazelton, B. J. (Author)
- Hindson, L. (Author)
- Johnston-Hollitt, M. (Author)
- Jacobs, Daniel (Author)
- Kasper, J. C. (Author)
- Kratzenberg, E. (Author)
- Lenc, E. (Author)
- Lonsdale, C. J. (Author)
- Lynch, M. J. (Author)
- McWhirter, S. R. (Author)
- Mitchell, D. A. (Author)
- College of Liberal Arts and Sciences (Contributor)
- Digital object identifier: 10.1093/mnras/stu1368
- Identifier TypeInternational standard serial numberIdentifier Value2470-0053
- Identifier TypeInternational standard serial numberIdentifier Value2470-0045
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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., & Mitche (2014). WSCLEAN: an implementation of a fast, generic wide-field imager for radio astronomy. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 444(1), 606-619. http://dx.doi.org/10.1093/mnras/stu1368