1 code implementation • 31 Mar 2020 • Devansh Agarwal, D. R. Lorimer, M. P. Surnis, X. Pei, A. Karastergiou, G. Golpayegani, D. Werthimer, J. Cobb, M. A. McLaughlin, S. White, W. Armour, D. H. E. MacMahon, A. P. V. Siemion, G. Foster
Depending on the observing mode, this translates to peak flux sensitivities in the range 0. 14--0. 89~Jy.
Instrumentation and Methods for Astrophysics