The correlation calibration of PAPER-64 data

Author:

Gogo Tamirat G12,Ma Yin-Zhe12ORCID,Kittiwisit Piyanat12,Sievers Jonathan L13,Parsons Aaron R45,Pober Jonathan C6,Jacobs Daniel C7,Cheng Carina4,Kolopanis Matthew7ORCID,Liu Adrian89,Kohn Saul A10,Aguirre James E10ORCID,Ali Zaki S5,Bernardi Gianni111213,Bradley Richard F141516,DeBoer David R5,Dexter Matthew R5,Dillon Joshua S4ORCID,Klima Pat15,MacMahon David H E5,Moore David F10,Nunhokee Chuneeta D4,Walbrugh William P13,Walker Andre11

Affiliation:

1. School of Chemistry and Physics, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban, 4000, South Africa

2. NAOC-UKZN Computational Astrophysics Centre (NUCAC), University of KwaZulu-Natal, Durban, 4000, South Africa

3. Department of Physics, McGill University, 3600 University Street Montreal, QC H3A 2T8, Canada

4. Department of Astronomy, UC Berkeley, Berkeley, CA 94720, USA

5. Radio Astronomy Laboratory, UC Berkeley, Berkeley, CA 94720, USA

6. Department of Physics, Brown University, Providence, RI 02912, USA

7. School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA

8. Department of Physics and McGill Space Institute, McGill University, Montreal, QC H3A 2T8, Canada

9. CIFAR Azrieli Global Scholar, Gravity & the Extreme Universe Program, Canadian Institute for Advanced Research, 661 University Ave., Suite 505, Toronto, Ontario M5G 1M1, Canada

10. Department of Physics and Astronomy, U. Penn., Philadelphia PA 19104, USA

11. INAF-Istituto di Radioastronomia, via Gobetti 101, I-40129, Bologna, Italy

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

13. South African Radio Astronomy Observatory, Black River Park, 2 Fir Street, Observatory, Cape Town, 7925, South Africa

14. Department of Electrical and Computer Engineering, U. Virginia, Charlottesville VA 22904, USA

15. National Radio Astronomy Obs., Charlottesville VA 22904, USA

16. Department of Astronomy, U. Virginia, Charlottesville VA 22904, USA

Abstract

ABSTRACT Observation of redshifted 21-cm signal from the Epoch of Reionization (EoR) is challenging due to contamination from the bright foreground sources that exceed the signal by several orders of magnitude. Removal of this very high foreground relies on accurate calibration to keep the intrinsic property of the foreground with frequency. Commonly employed calibration techniques for these experiments are the sky model-based and the redundant baseline-based calibration approaches, which can suffer from sky-modelling error and array redundancy imperfection respectively. In this work, we introduce the hybrid correlation calibration (CorrCal) scheme, which aims to bridge the gap between redundant and sky-based calibration by relaxing redundancy of the array and including sky information into the calibration formalisms. We apply the CorrCal to the data of Precision Array for Probing the Epoch of Reionization (PAPER) experiment, which was pre-calibrated using redundant baseline calibration. We show about $6\%$ suppression at the bin right on the horizon limit of the foreground wedge-like structure, relative to the pre-calibrated power spectra. This small improvement of the foreground power spectra around the wedge limit could be suggestive of reduced spectral structure in the data after CorrCal calibration, which lays the foundation for future improvement of the calibration algorithm and implementation method.

Funder

University of KwaZulu-Natal

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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