activity
19992025
most citedThe NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background

1.5k citations · 9.6k across the 78 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

6 papers · 2 filters

astro-ph2003

Detection of Sagittarius A* at 330 MHz with the Very Large Array

Michael E. Nord, T. Joseph W. Lazio, Namir E. Kassim +2

We report the detection of Sagittarius A*, the radio source associated with our Galaxy's central massive black hole, at 330 MHz with the Very Large Array. Implications for the spec…

astro-ph2003★ 139 cited

Pulsar Parallaxes at 5 GHz with the Very Long Baseline Array

S. Chatterjee, J. M. Cordes, W. H. T. Vlemmings +3

We present the first pulsar parallaxes measured with phase-referenced pulsar VLBI observations at 5 GHz. Due to the steep spectra of pulsars, previous astrometric measurements have…

astro-ph2003

A Deep, High-Resolution Survey at 74 MHz

A. S. Cohen, H. J. A. Rottgering, M. J. Jarvis +2

We present a 74 MHz survey of a 165 square degree region located near the north galactic pole. This survey has an unprecedented combination of both resolution (25'' FWHM) and sensi…

astro-ph2003

A Low Frequency Survey of the Galactic Plane Near l=11 degrees: Discovery of Three New Supernova Remnants

C. L. Brogan, K. E. Devine, T. J. Lazio +5

We have imaged a 1 deg^2 field centered on the known Galactic supernova remnant (SNR) G11.2-0.3 at 74, 330, and 1465 MHz with the Very Large Array radio telescope (VLA) and 235 MHz…

astro-ph2003

Nonthermal Emission from the Arches Cluster (G0.121+0.017) and the Origin of -ray Emission from 3EG J1746-2851

F. Yusef-Zadeh, M. Nord, M. Wardle +3

High resolution VLA observations of the Arches cluster near the Galactic center show evidence of continuum emission at 3.6, 6, 20 and 90cm. The continuum emission at 90cm is…

astro-ph2003★ 66 cited

NE2001. II. Using Radio Propagation Data to Construct a Model for the Galactic Distribution of Free Electrons

J. M. Cordes, T. J. W. Lazio

In Paper I we present a new model for the Galactic distribution of free electrons. In this paper we describe the input data and methodology for determining the structure and parame…