Direction-dependent calibration with image-domain gridding

Aims. Wide-field images made by radio interferometers are invariably affected by direction-dependent systematic effects such as the ionosphere or the beam pattern. Calibration along a set of discrete directions in the sky is the default technique to estimate and correct these systematic errors. However, additional processing such as smoothing and mosaicing are required to reconcile the step wise variation of the estimated systematic errors at the edges of the discrete directions (facets). Methods. We overcome the discrete nature of direction-dependent calibration by using image-domain gridding as the model for the calibration. Instead of discrete directions in the sky, calibration is performed using a basis that represents a set of sub-grids in the Fourier space. This automatically removes the need for extra operations to recover the wide-field systematics error model without any discontinuity. Results. We provide results based on LOFAR data where we compare the traditional facet-based (discrete directional gains) calibration with the proposed approach. The comparison shows improved image quality, mainly because of the physical plausibility of the proposed approach as opposed to using a piecewise constant model for direction-dependent systematic errors.

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2026-03-17
DOI
https://doi.org/10.1051/0004-6361/202558272/pdf
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
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article

Direction-dependent calibration with image-domain gridding

Springer Link (Chiba Institute of Technology)
Radio Astronomy Observations and Technology
article

Direction-dependent calibration with image-domain gridding

article en

Abstract

Aims. Wide-field images made by radio interferometers are invariably affected by direction-dependent systematic effects such as the ionosphere or the beam pattern. Calibration along a set of discrete directions in the sky is the default technique to estimate and correct these systematic errors. However, additional processing such as smoothing and mosaicing are required to reconcile the step wise variation of the estimated systematic errors at the edges of the discrete directions (facets). Methods. We overcome the discrete nature of direction-dependent calibration by using image-domain gridding as the model for the calibration. Instead of discrete directions in the sky, calibration is performed using a basis that represents a set of sub-grids in the Fourier space. This automatically removes the need for extra operations to recover the wide-field systematics error model without any discontinuity. Results. We provide results based on LOFAR data where we compare the traditional facet-based (discrete directional gains) calibration with the proposed approach. The comparison shows improved image quality, mainly because of the physical plausibility of the proposed approach as opposed to using a piecewise constant model for direction-dependent systematic errors.

Springer Link (Chiba Institute of Technology)
Openalex Percentile: Top 47%
Radio Astronomy Observations and Technology
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Direction-dependent calibration with image-domain gridding · Springer Link (Chiba Institute of Technology) (2026) | TGRS Research Map | TGRS