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Published May 2022 | Accepted Version + Published
Journal Article Open

MeqSilhouette v2: spectrally resolved polarimetric synthetic data generation for the event horizon telescope

Abstract

We present MeqSilhouette v2.0 (MeqSv2), a fully polarimetric, time-and frequency-resolved synthetic data generation software for simulating millimetre (mm) wavelength very long baseline interferometry (VLBI) observations with heterogeneous arrays. Synthetic data are a critical component in understanding real observations, testing calibration and imaging algorithms, and predicting performance metrics of existing or proposed sites. MeqSv2 applies physics-based instrumental and atmospheric signal corruptions constrained by empirically derived site and station parameters to the data. The new version is capable of applying instrumental polarization effects and various other spectrally resolved effects using the Radio Interferometry Measurement Equation (RIME) formalism and produces synthetic data compatible with calibration pipelines designed to process real data. We demonstrate the various corruption capabilities of MeqSv2 using different arrays, with a focus on the effect of complex bandpass gains on closure quantities for the EHT at 230 GHz. We validate the frequency-dependent polarization leakage implementation by performing polarization self-calibration of synthetic EHT data using PolSolve. We also note the potential applications for cm-wavelength VLBI array analysis and design and future directions.

Additional Information

© 2022 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2022 February 23. Received 2022 February 23; in original form 2021 November 25. Published: 26 February 2022. We thank Benna Hugo and André Offringa for discussions on WSCLEAN and Mareki Honma for his valuable comments. IN and RPD acknowledge support from the New Scientific Frontiers with Precision Radio Interferometry group grant awarded by the South African Radio Astronomy Observatory (SARAO), which is a facility of the National Research Foundation (NRF), an agency of the Department of Science and Innovation (DSI). IN, RPD, and OS acknowledge funding by the South African Research Chairs Initiative of the DSI/NRF. IMV acknowledges support from Research Project PID2019-108995GB-C22 of Ministerio de Ciencia e Innovación (Spain) and from the GenT Project CIDEGENT/2018/021 of Generalitat Valenciana (Spain). FR, MJ, JD, MM, and HF acknowledge support from the ERC Synergy Grant 'BlackHoleCam: Imaging the Event Horizon of Black Holes' (Grant 610058). FO and DP acknowledge support from the NSF PIRE grant OISE-1743747. MW and LB were supported by the Black Hole Initiative at Harvard University, which is funded by grants from the John Templeton Foundation and the Gordon and Betty Moore Foundation to Harvard University. KLB acknowledges support from the MSIP2: NSF Award 2034306. GB acknowledges support from the Ministero degli Affari Esteri della Cooperazione Internazionale - Direzione Generale per la Promozione del Sistema Paese Progetto di Grande Rilevanza ZA18GR02 and the National Research Foundation of South Africa (Grant Number 113121) as part of the ISARP RADIOSKY2020 Joint Research Scheme. Data Availability: MEQSV2 is open source and publicly available on GitHub at https://github.com/rdeane/MeqSilhouette. Its documentation can be found at https://meqsilhouette.readthedocs.io. Bugs and other issues can be reported by creating an issue on the repository. The data underlying this article will be shared on reasonable request to the corresponding author.

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Accepted Version - 2202.11478.pdf

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Additional details

Created:
August 22, 2023
Modified:
October 23, 2023