activity
20102015
most citedNew Black Widows and Redbacks in the Galactic Field

41 citations · 70 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2015★ 1 cited

Observations of Radio Giant Pulses with GAVRT

Glenn Jones

Radio giant pulses provide a unique opportunity to study the pulsar radio emission mechanism in exquisite detail. Previous studies have revealed a wide range of properties and phen…

astro-ph.HE2011★ 1 cited

Testing Gravity Theories In The Radiative Regime Using Pulsar Timing Arrays

K. J. Lee

General relativity has predicted the existence of gravitational waves (GW), which are waves of the distortions of space-time with two degrees of polarization and the propagation sp…

astro-ph.HE2011★ 2 cited

Constraining pulsar gap models with the light-curve and flux properties of the gamma-ray pulsar population

Marco Pierbattista, Isabelle Grenier, Alice Harding +1

We compare population synthesis results for inner and outer magnetosphere emission models with the various characteristics measured in the first LAT pulsar catalogue for both the r…

astro-ph.HE2011★ 41 cited

New Black Widows and Redbacks in the Galactic Field

Mallory S. E. Roberts, Fermi Pulsar Search Consortium, GBT Drift Scan Survey Collaboration

There has recently been a large increase in the number of known eclipsing radio millisecond pulsars in the Galactic field, many of which are associated with Fermi gamma-ray sources…

astro-ph.IM2011

Pulsar Science with the Green Bank 43m Telescope

M. B. Mickaliger, M. A. McLaughlin, D. R. Lorimer +5

The 43m telescope at the NRAO site in Green Bank, WV has recently been outfitted with a clone of the Green Bank Ultimate Pulsar Processing Instrument (GUPPI \cite{Ransom:2009}) bac…

astro-ph.HE2011★ 8 cited

Pulsar Timing Arrays and their Applications

R. N. Manchester

Millisecond pulsars are intrinsically very stable clocks and precise measurement of their observed pulse periods can be used to study a wide variety of astrophysical phenomena. In…

astro-ph.GA2010★ 14 cited

Blind surveys for radio pulsars and transients

D. R. Lorimer

The main reasons for searching for pulsars are to: (i) get an accurate census of the neutron star population and its origin and evolution; (ii) connect neutron stars to other stell…

astro-ph.HE2010

Pulsar Timing with the Fermi LAT

Paul S. Ray, Matthew Kerr, Damien Parent +1

We present an overview of precise pulsar timing using data from the Large Area Telescope (LAT) on Fermi. We describe the analysis techniques including a maximum likelihood method f…

astro-ph.HE2010★ 2 cited

Observations and Modeling of Gamma-ray Millisecond Pulsars seen with the Fermi LAT

Tyrel J. Johnson, Christo Venter, Alice K. Harding +1

We present a summary of gamma-ray millisecond pulsar (MSP) observations with the Fermi Large Area Telescope. The radio and gamma-ray light curves of these MSPs have been modeled in…

astro-ph.IM2010★ 1 cited

Pulsars with the Australian Square Kilometre Array Pathfinder

I. H. Stairs, M. J. Keith, Z. Arzoumanian +33

The Australian Square Kilometre Array Pathfinder (ASKAP) is a 36-element array with a 30-square-degree field of view being built at the proposed SKA site in Western Australia. We a…

astro-ph.HE2010

Neutron Star Astronomy with the HST

R. P. Mignani

Since its launch in 1990, HST has played a leading role in optical studies of isolated neutron stars, both radio-loud pulsars and radio-silent ones, paving the way to follow-up obs…

astro-ph.HE2010

On Energy- Angular Momentum- Loss and Pulsar Spark Gaps

Aldo Treves, Maura Pilia, Marcos Lopez Moya

The neutron star spin down imposes a balance between the energy and angular momentum (E/L) losses of a pulsar. This translates into constraints on the region of emission. The E/L b…