activity
19962023
most citedPSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

1.8k citations · 21k across the 177 of their papers we have counts for

collaborators
Showing 2012Show all

9 papers · 1 filter

astro-ph.HE2012★ 115 cited

Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations

H. J. Pletsch, L. Guillemot, H. Fehrmann +150

Millisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "…

astro-ph.HE2012★ 51 cited

Radio Detection of the Fermi LAT Blind Search Millisecond Pulsar J1311-3430

P. S. Ray, S. M. Ransom, C. C. Cheung +15

We report the detection of radio emission from PSR J1311-3430, the first millisecond pulsar discovered in a blind search of Fermi Large Area Telescope (LAT) gamma-ray data. We dete…

astro-ph.IM2012★ 65 cited

A wide-band, active antenna system for long wavelength radio astronomy

Brian C. Hicks, Nagini Paravastu-Dalal, Kenneth P. Stewart +9

We describe an "active" antenna system for HF/VHF (long wavelength) radio astronomy that has been successfully deployed 256-fold as the first station (LWA1) of the planned Long Wav…

astro-ph.IM2012★ 34 cited

The Long Wavelength Array Software Library

Jayce Dowell, Daniel Wood, Kevin Stovall +3

The Long Wavelength Array Software Library (LSL) is a Python module that provides a collection of utilities to analyze and export data collected at the first station of the Long Wa…

astro-ph.HE2012★ 49 cited

PSR J1838-0537: Discovery of a young, energetic gamma-ray pulsar

H. J. Pletsch, L. Guillemot, B. Allen +12

We report the discovery of PSR J1838-0537, a gamma-ray pulsar found through a blind search of data from the Fermi Large Area Telescope (LAT). The pulsar has a spin frequency of 6.9…

astro-ph.IM2012★ 1 cited

First Light for the First Station of the Long Wavelength Array

G. B. Taylor, S. W. Ellingson, N. E. Kassim +32

The first station of the Long Wavelength Array (LWA1) was completed in April 2011 and is currently performing observations resulting from its first call for proposals in addition t…