Cygnus A jointly calibrated and imaged via non-convex optimisation from VLA data

TL;DR

This paper introduces a novel non-convex optimization method for joint calibration and imaging in radio interferometry, improving resolution and fidelity of radio maps by promoting sparsity with a log-sum prior, demonstrated on Cygnus A data.

Contribution

It proposes a new sparsity-promoting prior and an iterative non-convex optimization approach for joint calibration and imaging in radio interferometry, enhancing image quality.

Findings

Enhanced data fidelity and resolution in radio maps.

Successful detection of background sources near Cygnus A.

Effective modeling of direction-dependent antenna gains.

Abstract

Radio interferometric (RI) data are noisy under-sampled spatial Fourier components of the unknown radio sky affected by direction-dependent antenna gains. Failure to model these antenna gains accurately results in a radio sky estimate with limited fidelity and resolution. The RI inverse problem has been recently addressed via a joint calibration and imaging approach which consists in solving a non-convex minimisation task, involving suitable priors for the DDEs, namely temporal and spatial smoothness, and sparsity for the unknown radio map via an $\ell_1$-norm prior, in the context of realistic RI simulations. Building on these developments, we propose to promote sparsity of the radio map via a log-sum prior, enforcing sparsity more strongly than the $\ell_1$-norm. The resulting minimisation task is addressed via a sequence of non-convex minimisation tasks composed of re-weighted $\ell_1$ image priors, which are solved approximately. We demonstrate the efficiency of the approach on RI observations of the celebrated radio galaxy Cygnus~A obtained with the Karl G. Jansky Very Large Array at X, C, and S bands. More precisely, we showcase that the approach enhances data fidelity significantly while achieving high resolution high dynamic range radio maps, confirming the suitability of the priors considered for the unknown DDEs and radio image. As a clear qualitative indication of the high fidelity achieved by the data and the proposed approach, we report the detection of three background sources in the vicinity of Cyg~A, at S band.