MeqSilhouette v2: Spectrally resolved polarimetric synthetic data generation for the event horizon telescope
Author
Natarajan, I.Deane, R.
Martí-Vidal, I.
Roelofs, F.
Janssen, M.
Wielgus, M.
Blackburn, L.
Blecher, T.
Perkins, S.
Smirnov, O.
Davelaar, J.
Moscibrodzka, M.
Chael, A.
Bouman, K.L.
Kim, J.-Y.
Bernardi, G.
Van Bemmel, I.
Falcke, H.
Özel, F.
Psaltis, D.
Affiliation
Department of Astronomy and Steward Observatory, University of ArizonaIssue Date
2022
Metadata
Show full item recordPublisher
Oxford University PressCitation
Natarajan, I., Deane, R., Martí-Vidal, I., Roelofs, F., Janssen, M., Wielgus, M., Blackburn, L., Blecher, T., Perkins, S., Smirnov, O., Davelaar, J., Moscibrodzka, M., Chael, A., Bouman, K. L., Kim, J.-Y., Bernardi, G., Van Bemmel, I., Falcke, H., Özel, F., & Psaltis, D. (2022). MeqSilhouette v2: Spectrally resolved polarimetric synthetic data generation for the event horizon telescope. Monthly Notices of the Royal Astronomical Society.Rights
Copyright © 2022 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.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. © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.Note
Immediate accessISSN
0035-8711Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1093/mnras/stac531