T CrB: Radio Observations during the 2016–2017 “Super-active” State

We thank the anonymous referee for insightful comments and criticisms, which led to an improved version of this manuscript. We appreciate the useful conversations about T CrB, CVs, and accretion at the Stellar Remnants at the Junction meeting and the Conference on Shocks and Particle Acceleration in Novae and Supernovae. We thank Dr. Bob Zavala and the USNO review board for their helpful comments on this manuscript. We acknowledge support from NASA award NNX14AQ36G. J. L. S. and J. H. S. W. were funded in part by NSF award AST-1211778. L.C. acknowledges support from a Cottrell Scholarship of the Research Corporation and NSF AST-1751874. We thank the NRAO for the generous allocation of VLA time for our observations. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. We acknowledge with thanks the variable star observations from the AAVSO International Database (Kafka 2018) contributed by observers worldwide and used in this research. This research made use of SciPy (Oliphant 2007), an open-source library of numerical routines for scientific computing available at http://www.scipy.org; NumPy (van der Walt et al. 2011), the fundamental package for scientific computing with Python; APLpy (Robitaille & Bressert 2012), an open-source plotting package for Python hosted at http://aplpy.github.com; and Astropy (Astropy Collaboration 2013, 2018), a community-developed core Python package for Astronomy available at http://www.astropy.org. The figures in this manuscript were made using the matplotlib 2D graphics package for Python (Hunter 2007).