GBT19B-320

Timing Observations of GBNCC Discovered Pulsars

Abstract

We propose prime focus observations of five pulsars discovered in the GBNCC survey. One is a relativistic binary and another a long-orbital-period binary, and the other four are rotating radio transients. We request a month of high cadence observations followed by monthly observations. The observations of J1800/J2038 can be done at either 820 or 350. The other observations must be done at 350.

Investigators

Name	Institution
Maura McLaughlin *	West Virginia University
Gabriella Agazie	West Virginia University; Wisconsin at Milwaukee, University of
Michael Mingyar	West Virginia University
Joseph Swiggum	West Virginia University; Wisconsin at Milwaukee, University of
Ryan Lynch	Green Bank Observatory
Emmanuel Fonseca	British Columbia, University of; McGill University; West Virginia University
Megan DeCesar	George Mason University
William Fiore	British Columbia, University of; West Virginia University
Kevin Stovall	National Radio Astronomy Observatory; New Mexico, University of; Texas at Brownsville, University of
Ingrid Stairs	British Columbia, University of
David Kaplan	Wisconsin at Milwaukee, University of
Scott Ransom	National Radio Astronomy Observatory; Virginia, University of
Joeri van Leeuwen	Netherlands Institute for Radio Astronomy
Alexander McEwen	Wisconsin at Milwaukee, University of

* indicates the PI