We propose to observe 2 binary millisecond pulsars currently being monitored by NANOGrav using high time/frequency resolution. We have found the presence of well characterized "scintillation arcs", which are parabolic intensity features in the Fourier transform of dynamic spectra. Our objective is to analyze the variations in the scintillation arc curvatures for these two pulsars over one orbital phase. Recent work demonstrates that scintillation arcs can be used to directly measure key features of the interstellar medium and orbital geometry, especially if independent estimates of the pulsar distance and proper motion are known through high-precision timing of PTA data. By combining arc-based measurements of geometry with radio-timing measurements, we will be able to derive intrinsic properties of orbital systems, such as the pulsar and companion masses. We request to observe each source with the PF/820-MHz receiver. As described in the proposal, for each of the two pulsars, we seek 2-hour observing sessions, allocating 18 randomly scheduled sessions over the course of one observing year. This totals to an observing time of 36 hrs per source, making the aggregate of 72 hrs for this program.
Name | Institution |
---|---|
Swarali Shivraj Patil * | West Virginia University |
Emmanuel Fonseca | British Columbia, University of; McGill University; West Virginia University |
Joseph Glaser | West Virginia University |
Megan DeCesar | George Mason University |
Natalia Lewandowska | New York at Oswego, State University of |
James McKee | Hull, University of |
Jim Cordes | Cornell University |
Jacob Turner | Green Bank Observatory; West Virginia University |
Stella Ocker | Carnegie Institute of Washington; California Institute of Technology |
Benetge Perera | National Astronomy and Ionosphere Center ; West Virginia University; Florida, University of Central |
Thankful Cromartie | Cornell University; Virginia, University of; Naval Research Laboratory |
Maura McLaughlin | West Virginia University |
Michael Lam | Cornell University; Rochester Institute of Technology; West Virginia University; SETI Institute |
Daniel Stinebring | Oberlin College |
Robert Main | McGill University |
Ingrid Stairs | British Columbia, University of |
Lydia Guertin | Academia Sinica |
Timothy Dolch | Cornell University; Oberlin College; Hillsdale College |
* indicates the PI