Primary beam effects of radio astronomy antennas – I. Modelling the Karl G. Jansky Very Large Array (VLA) L-band beam using holography-Reference-Cited by-同舟云学术

Primary beam effects of radio astronomy antennas – I. Modelling the Karl G. Jansky Very Large Array (VLA) L-band beam using holography

Author:

Iheanetu K¹,Girard J N¹²,Smirnov O¹³,Asad K M B¹³⁴,de Villiers M³,Thorat K¹³,Makhathini S¹³,Perley R A¹⁵

Affiliation:

1. Department of Physics and Electronics, Rhodes University, PO Box 94, Grahamstown 6140, South Africa

2. AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France

3. South African Radio Astronomy Observatory, 3rd Floor, The Park, Park Road, Pinelands, Cape Town 7405, South Africa

4. Department of Physics and Astronomy, University of the Western Cape, Bellville, Cape Town 7535, South Africa

5. National Radio Astronomy Observatory, P.O. Box 87801, USA

Funder

National Research Foundation

Sorbonne Paris Cité

European Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference20 articles.

Cited by 13 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

2. Mining mini-halos with MeerKAT I. Calibration and imaging;Monthly Notices of the Royal Astronomical Society;2023-02-03

4. Quality Assessment Tool for SKA Continuum Imaging Pipelines;2022 3rd URSI Atlantic and Asia Pacific Radio Science Meeting (AT-AP-RASC);2022-05-29