CASCA is pleased to announce that the recipient of the 2017 Peter G. Martin award is Dr. Ingrid Stairs of the University of British Columbia.
After receiving her PhD in 1998 from Princeton University, Dr. Stairs went to the University of Manchester from 1998 to 2000 to pursue postdoctoral work. She then continued her research at the National Radio Astronomy Observatory from 2000 to 2002 as a Jansky Fellow. She joined the faculty at UBC in 2002 and became a tenured professor in 2007. The Canadian Institute for Advanced Research appointed her as Senior Fellow in 2014.
Dr. Stairs is one of world’s experts on pulsars and has made significant contributions to radio astronomy instrumentation. She developed the novel Princeton Mark IV back-end instrument for use at the Arecibo telescope for high-precision timing of relativistic pulsars that was used in the discovery of general-relativistic orbital decay of the binary pulsar PSR B1534+12. She made the first measurement of the Shapiro delay, which continues to enable multiple new tests of General Relativity. She is involved in the development of instrumentation for the upcoming CHIME radio telescope that will observe pulsars as well as the cosmological distribution of hydrogen. She is the Observational Coordinator for the North American Nanohertz Observatory for Gravitational Waves (NANOGrav).
CASCA congratulates Dr. Stairs on the receipt of the 2017 Martin Award for her fundamental contributions to radio astronomy instrumentation and the understanding of pulsars that have shed new light on General Relativity.