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- Publications
- Influence
Fast Radio Burst Discovered in the Arecibo Pulsar ALFA Survey
- L. Spitler, J. Cordes, +30 authors H. Fehrmann
- Physics
- 10 April 2014
Recent work has exploited pulsar survey data to identify temporally isolated, millisecond-duration radio bursts with large dispersion measures (DMs). These bursts have been interpreted as arising… Expand
Pulsar J0453+1559: A Double Neutron Star System with a Large Mass Asymmetry
- J. G. Martinez, K. Stovall, +6 authors A. Ridolfi
- Physics
- 29 September 2015
To understand the nature of supernovae and neutron star (NS) formation, as well as binary stellar evolution and their interactions, it is important to probe the distribution of NS masses. Until now,… Expand
An Eccentric Binary Millisecond Pulsar in the Galactic Plane
- D. Champion, S. Ransom, +28 authors W. Vlemmings
- Physics, Medicine
- Science
- 15 May 2008
Binary pulsar systems are superb probes of stellar and binary evolution and the physics of extreme environments. In a survey with the Arecibo telescope, we have found PSR J1903+0327, a radio pulsar… Expand
Timing stability of millisecond pulsars and prospects for gravitational-wave detection
- J. Verbiest, M. Bailes, +11 authors X. You
- Physics
- 3 August 2009
Analysis of high-precision timing observations of an array of " 20 millisecond pulsars (a socalled “timing array”) may ultimately result in the detection of a stochastic gravitational-wave… Expand
Upper bounds on the low-frequency stochastic gravitational wave background from pulsar timing observations: current limits and future prospects
Using a statistically rigorous analysis method, we place limits on the existence of an isotropic stochastic gravitational wave background using pulsar timing observations. We consider backgrounds… Expand
The stochastic background: scaling laws and time to detection for pulsar timing arrays
- X. Siemens, J. Ellis, F. Jenet, J. Romano
- Physics
- 14 May 2013
We derive scaling laws for the signal-to-noise ratio of the optimal cross-correlation statistic, and show that the large power-law increase of the signal-to-noise ratio as a function of the the… Expand
Measurement of Orbital Decay in the Double Neutron Star Binary PSR B2127+11C
- B. A. Jacoby, P. B. Cameron, F. Jenet, S. Anderson, R. Murty, S. Kulkarni
- Physics
- 15 May 2006
We report the direct measurement of orbital period decay in the double neutron star pulsar system PSR B2127+11C in the globular cluster M15 at the rate of (-3.95 ± 0.13) × 10-12, consistent with the… Expand
The Green Bank Northern Celestial Cap Pulsar Survey - I: Survey Description, Data Analysis, and Initial Results
- K. Stovall, R. Lynch, +29 authors B. Wells
- Physics
- 19 June 2014
We describe an ongoing search for pulsars and dispersed pulses of radio emission, such as those from rotating radio transients (RRATs) and fast radio bursts (FRBs), at 350 MHz using the Green Bank… Expand
Limits on the Stochastic Gravitational Wave Background from the North American Nanohertz Observatory for Gravitational Waves
- P. Demorest, R. Ferdman, +24 authors W. Zhu
- Physics
- 31 January 2012
We present an analysis of high-precision pulsar timing data taken as part of the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) project. We have observed 17 pulsars for a… Expand
The NANOGrav Nine-year Data Set: Observations, Arrival Time Measurements, and Analysis of 37 Millisecond Pulsars
- Z. Arzoumanian, A. Brazier, +41 authors W. Zhu
- Physics
- 28 May 2015
We present high-precision timing observations spanning up to nine years for 37 millisecond pulsars monitored with the Green Bank and Arecibo radio telescopes as part of the North American Nanohertz… Expand
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