Trajectory-based RFI subtraction and calibration for radio interferometry

Author:

Finlay Chris1234ORCID,Bassett Bruce A2354,Kunz Martin1,Oozeer Nadeem346

Affiliation:

1. Département de Physique Théorique and Center for Astroparticle Physics, Université de Genève , 24 quai Ernest Ansermet, 1211 Genève 4, Switzerland

2. Department of Pure and Applied Mathematics, University of Cape Town , 7700 Cape Town, South Africa

3. African Institute for Mathematical Sciences , 6 Melrose Road, Muizenberg, 7945 Cape Town, South Africa

4. South African Radio Astronomy Observatory (SARAO) , 2 Fir Street, Observatory, 7925 Cape Town, South Africa

5. South African Astronomical Observatory , Observatory Road, Observatory, 7925 Cape Town, South Africa

6. Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University , P.O. Box 94, 6140 Makhanda, South Africa

Abstract

ABSTRACT Radio interferometry calibration and radio frequency interference (RFI) removal are usually done separately. Here we show that jointly modelling the antenna gains and RFI has significant benefits when the RFI follows precise trajectories, such as for satellites. One surprising benefit is improved calibration solutions, by leveraging the RFI signal itself. We present trajectory-based RFI subtraction and calibration (tabascal), a new algorithm that jointly models the RFI and calibration parameters in visibilities. We test tabascal on simulated MeerKAT calibration observations contaminated by satellite-based RFI. We obtain gain estimates that are both unbiased and up to an order of magnitude better constrained compared to uncontaminated data. When combined with an ad hoc RFI subtraction scheme, tabascal solutions can be further applied to an adjacent target observation: 5 min of calibration data results in an image with about a third the noise achieved when using flagging alone. The recovered flux distribution of RFI subtracted data was on par with uncontaminated data. In contrast, RFI flagging alone resulted in a higher detection threshold and consistent underestimation of source fluxes. For a mean RFI amplitude of 17 Jy, using RFI subtraction leads to less than 1 per cent loss of data compared to 75 per cent data loss from an ideal 3σ flagging algorithm, a very significant increase in data available for science analysis. Although we have examined the case of satellite RFI, tabascal should work for any RFI moving on parametrizable trajectories, relative to the phase centre, such as planes and/or objects fixed to the ground.

Funder

Swiss National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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