Revisiting the radio interferometer measurement equation. III. Addressing direction-dependent effects in 21 cm WSRT observations of 3C 147
Oleg M. Smirnov

TL;DR
This paper demonstrates a RIME-based calibration method for WSRT 21 cm observations of 3C 147, achieving high dynamic range imaging by effectively addressing direction-dependent effects and improving calibration accuracy.
Contribution
It provides a practical implementation of differential gains within the RIME framework for high-dynamic range calibration, enabling better correction of DDEs in radio interferometry.
Findings
Achieved a 1.6 million dynamic range image of 3C 147
Successfully used differential gains to correct DDEs and improve image quality
Sources as faint as 2 mJy can serve as calibration beacons
Abstract
Papers I and II of this series have extended the radio interferometry measurement equation (RIME) formalism to the full-sky case, and provided a RIME-based description of calibration and the problem of direction-dependent effects (DDEs). This paper aims to provide a practical demonstration of a RIME-based approach to calibration, via an example of extremely high-dynamic range calibration of WSRT observations of 3C 147 at 21 cm, with full treatment of DDEs. A version of the RIME incorporating differential gains has been implemented in MeqTrees, and applied to the 3C 147 data. This was used to perform regular selfcal, then solve for interferometer-based errors and for differential gains. The resulting image of the field around 3C 147 is thermal noise-limited, has a very high dynamic range (1.6 million), and none of the off-axis artefacts that plague regular selfcal. The differential…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Soil Moisture and Remote Sensing · Radio Wave Propagation Studies
