Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWA
W Li, JC Pober, BJ Hazelton, N Barry, MF Morales, I Sullivan, AR Parsons, ZS Ali, JS Dillon, AP Beardsley, JD Bowman, F Briggs, R Byrne, P Carroll, B Crosse, D Emrich, A Ewall-Wice, L Feng, TMO Franzen, JN Hewitt Show all
The Astrophysical Journal | IOP PUBLISHING LTD | Published : 2018
Awarded by NSF
Awarded by NSF Astronomy and Astrophysics Postdoctoral Fellowship
W.L., J.C.P., B.J.H., N.B., M.F.M., and I.S. would like to acknowledge the support from NSF grant nos. 1613040, 1613855, and 1506024. J.S.D. acknowledges the support of NSF award no. 1701536. A.P.B. acknowledges the NSF Astronomy and Astrophysics Postdoctoral Fellowship under award AST-1701440. This scientific work makes use of the Murchison Radio-astronomy Observatory, operated by CSIRO. We acknowledge the Wajarri Yamatji people as the traditional owners of the Observatory site. Support for the operation of the MWA is provided by the Australian Government (NCRIS), under a contract to Curtin University administered by Astronomy Australia Limited. We acknowledge the Pawsey Supercomputing Centre, which is supported by the Western Australian and Australian Governments. This research was conducted using computation resources and services at the Center for Computation and Visualization, Brown University. We acknowledge Greg Rowbotham for providing the picture of MWA Phase II tiles.