The FHD polarised imaging pipeline: A new approach to widefield interferometric polarimetry
Abstract
We describe a new polarised imaging pipeline implemented in the FHD software package. The pipeline is based on the optimal mapmaking imaging approach and performs horizon-to-horizon image reconstruction in all polarisation modes. We discuss the formalism behind the pipeline's polarised analysis, describing equivalent representations of the polarised beam response, or Jones matrix. We show that, for arrays where antennas have uniform polarisation alignments, defining a non-orthogonal instrumental polarisation basis enables accurate and efficient image reconstruction. Finally, we present a new calibration approach that leverages widefield effects to perform fully polarised calibration. This analysis pipeline underlies the analysis of Murchison Widefield Array data in Byrne et al. (2022, MNRAS, 510, 2011).
Additional Information
© The Author(s), 2022. Published by Cambridge University Press on behalf of the Astronomical Society of Australia. Received 25 January 2022; revised 30 March 2022; accepted 13 April 2022. Published online by Cambridge University Press: 13 May 2022. We would like to thank James Aguirre, Zachary Martinot, and Daniel Mitchell for conversations that contributed to this work. Thank you to Yuping Huang for assisting with revision of this paper. This work was directly supported by National Science Foundation (NSF) grant 1613855.Attached Files
Submitted - 2201.10653.pdf
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Additional details
- Alternative title
- The FHD Polarized Imaging Pipeline: A New Approach to Widefield Interferometric Polarimetry
- Eprint ID
- 114518
- DOI
- 10.1017/pasa.2022.21
- Resolver ID
- CaltechAUTHORS:20220428-212301062
- NSF
- AST-1613855
- Created
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2022-04-28Created from EPrint's datestamp field
- Updated
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2022-07-20Created from EPrint's last_modified field