A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes
E D Barr(Max Planck Institute for Radio Astronomy), Andrea Possenti(West Virginia University), D. J. Champion(Commonwealth Scientific and Industrial Research Organisation), A. Ridolfi(Osservatorio Astronomico di Cagliari), Norbert Wex(Max Planck Institute for Radio Astronomy), S. M. Ransom(National Radio Astronomy Observatory), Cristina Pallanca(Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna), J. Behrend(Max Planck Institute for Radio Astronomy), A. Corongiu(Osservatorio Astronomico di Cagliari), Yunpeng Men(Max Planck Institute for Radio Astronomy), P V Padmanabh(Leibniz University Hannover), Mario Cadelano(Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna), M. Geyer(South African Radio Astronomy Observatory), V. Venkatraman Krishnan(ARC Centre of Excellence for All-sky Astrophysics), B. W. Stappers(University of Manchester), M. Burgay(West Virginia University), T. Gautam(Max Planck Institute for Radio Astronomy), M. Bailes(ARC Centre of Excellence for Gravitational Wave Discovery), W Chen(Max Planck Institute for Radio Astronomy), C.‐H. Rosie Chen(Max Planck Institute for Radio Astronomy), P. C. C. Freire(Max Planck Institute for Radio Astronomy), Thomas M. Tauris(Max Planck Institute for Radio Astronomy), Arunima Dutta(Max Planck Institute for Radio Astronomy), S. Buchner(South African Radio Astronomy Observatory)
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