Pre-selection of the candidate fields for deep imaging of the epoch of reionization with SKA1-low

Author:

Zheng Qian1,Wu Xiang-Ping12,Guo Quan1,Johnston-Hollitt Melanie34,Shan Huanyuan15,Duchesne Stefan W4,Li Weitian6

Affiliation:

1. Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China

2. National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Beijing 100012, China

3. Curtin Institute for Computation, GPO Box U1987, Perth, WA 6845, Australia

4. International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, WA, Australia

5. University of Chinese Academy of Sciences, Beijing 100049, China

6. School of Physics and Astronomy, Shanghai Jiao Tong University, 800 Dongchuan Road, Shanghai 200240, China

Abstract

ABSTRACT The Square Kilometre Array (SKA) will be the first low-frequency instrument with the capability to directly image the structures of the epoch of reionization (EoR). Indeed, deep imaging of the EoR over five targeted fields of 20 sq deg each has been selected as the highest priority science objective for SKA1. Aiming at preparing for this highly challenging observation, we perform an extensive pre-selection of the ‘quietest’ and ‘cleanest’ candidate fields in the southern sky to be suited for deep imaging of the EoR using existing catalogues and observations over a broad frequency range. The candidate fields should meet a number of strict criteria to avoid contaminations from foreground structures and sources. The candidate fields should also exhibit both the lowest average surface brightness and smallest variance to ensure uniformity and high-quality deep imaging over the fields. Our selection eventually yields a sample of 7 ‘ideal’ fields of 20 sq deg in the southern sky that could be targeted for deep imaging of the EoR. Finally, these selected fields are convolved with the synthesized beam of SKA1-low stations to ensure that the effect of sidelobes from the far-field bright sources is also weak.

Funder

National Key Research and Development Program of China

National Natural Science Foundation of China

Center for Advanced Study, University of Illinois at Urbana-Champaign

Curtin University of Technology

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 1 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

1. A semi-analytical model for the formation and evolution of radio relics in galaxy clusters;Monthly Notices of the Royal Astronomical Society;2022-09-24

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