We propose to continue a pilot pulsar survey of the Galactic plane in a 25 square-deg region (5deg<=l<=10deg, 5<=b<= 10deg). We optimistically expect to discover 14+/-3 new pulsars in this pilot project, making it a worthwhile endeavor in its own right. We have an additional goal of empirically validating simulations suggesting that a larger GBT L-Band Galactic plane survey could discover ~500 new pulsars, ~50 of which would be millisecond pulsars. If these estimates are accurate then such a pulsar survey would be among the most successful ever performed, but radio frequency interference and other difficult-to-model effects are likely to reduce the actual yield, perhaps substantially. The pilot program that we propose here will allow us to confidently and optimally design a future large survey. We have thus far collected 1.5 hours of survey data, which has allowed us to test our data reduction pipeline. Continuing the pilot survey, and eventually completing a larger survey, will help to answer many outstanding questions in pulsar astronomy.
Name | Institution |
---|---|
Ryan Lynch * | Green Bank Observatory |
Gabriella Agazie | West Virginia University; Wisconsin at Milwaukee, University of |
David Kaplan | Wisconsin at Milwaukee, University of |
Megan DeCesar | George Mason University |
Benetge Perera | National Astronomy and Ionosphere Center ; West Virginia University; Florida, University of Central |
Scott Ransom | National Radio Astronomy Observatory; Virginia, University of |
Timothy Dolch | Cornell University; Oberlin College; Hillsdale College |
Alexander McEwen | Wisconsin at Milwaukee, University of |
Emilie Parent | Instituto de Ciencias del Espacio |
Olivia Young | Rochester Institute of Technology; West Virginia University |
Shawaiz Tabassum | West Virginia University; Abu Dhabi, New York University |
Vicky Kaspi | McGill University |
Jim Cordes | Cornell University |
Shami Chatterjee | Cornell University |
Fronefield Crawford | Franklin and Marshall College |
Joeri van Leeuwen | Netherlands Institute for Radio Astronomy |
William Fiore | British Columbia, University of; West Virginia University |
Rahul Sengar | Wisconsin at Milwaukee, University of |
* indicates the PI