activity
19962026
most citedShapiro delay measurement of a two solar mass neutron star

3.9k citations · 48.4k across the 396 of their papers we have counts for

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Showing astro-ph.GAShow all

31 papers · 1 filter

astro-ph.GA2023★ 22 cited

JWST uncovers helium and water abundance variations in the bulge globular cluster NGC 6440

Mario Cadelano, Cristina Pallanca, Emanuele Dalessandro +9

We used ultra-deep observations obtained with the NIRCam aboard the James Webb Space Telescope to explore the stellar population of NGC 6440: a typical massive, obscured and contam…

astro-ph.GA2023★ 68 cited

An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB

Amanda M. Cook, Mohit Bhardwaj, B. M. Gaensler +25

The CHIME/FRB project has detected hundreds of fast radio bursts (FRBs), providing an unparalleled population to probe statistically the foreground media that they illuminate. One…

astro-ph.GA2023★ 38 cited

The NANOGrav 12.5-year Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries

Zaven Arzoumanian, Paul T. Baker, Laura Blecha +75

Pulsar timing array collaborations, such as the North American Nanohertz Observatory for Gravitational Waves (NANOGrav), are seeking to detect nanohertz gravitational waves emitted…

astro-ph.GA2021★ 35 cited

The NANOGrav 11yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500Mpc

Zaven Arzoumanian, Paul T. Baker, Adam Brazier +54

Supermassive black hole binaries (SMBHBs) should form frequently in galactic nuclei as a result of galaxy mergers. At sub-parsec separations, binaries become strong sources of low-…

astro-ph.GA2020★ 4 cited

Multi-Messenger Gravitational Wave Searches with Pulsar Timing Arrays: Application to 3C66B Using the NANOGrav 11-year Data Set

Zaven Arzoumanian, Paul T. Baker, Adam Brazier +56

When galaxies merge, the supermassive black holes in their centers may form binaries and, during the process of merger, emit low-frequency gravitational radiation in the process. I…

astro-ph.GA2019★ 13 cited

Detection of pulses from the Vela pulsar at millimeter wavelengths with phased ALMA

Kuo Liu, Andre Young, Robert Wharton +20

We report on the first detection of pulsed radio emission from a radio pulsar with the ALMA telescope. The detection was made in the Band-3 frequency range (85-101 GHz) using ALMA…

astro-ph.GA2017★ 1 cited

A search for extragalactic pulsars in the Local Group galaxies IC 10 and Barnard's Galaxy

Hind Al Noori, Mallory S. E. Roberts, David Champion +3

As of today, more than 2500 pulsars have been found, nearly all in the Milky Way, with the exception of ~28 pulsars in the Small and Large Magellanic Clouds. However, there have be…

astro-ph.GA2015★ 71 cited

The NANOGrav Nine-year Data Set: Astrometric Measurements of 37 Millisecond Pulsars

Allison M. Matthews, David J. Nice, Emmanuel Fonseca +18

Using the nine-year radio-pulsar timing data set from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav), collected at Arecibo Observatory and the Green Ba…

astro-ph.GA2015★ 321 cited

The NANOGrav Nine-year Data Set: Limits on the Isotropic Stochastic Gravitational Wave Background

Zaven Arzoumanian, Adam Brazier, Sarah Burke-Spolaor +45

We compute upper limits on the nanohertz-frequency isotropic stochastic gravitational wave background (GWB) using the 9-year data release from the North American Nanohertz Observat…

astro-ph.GA2015★ 66 cited

NANOGrav Constraints on Gravitational Wave Bursts with Memory

Z. Arzoumanian, A. Brazier, S. Burke-Spolaor +39

Among efforts to detect gravitational radiation, pulsar timing arrays are uniquely poised to detect "memory" signatures, permanent perturbations in spacetime from highly energetic…

astro-ph.GA2014★ 134 cited

NANOGrav Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries in Circular Orbits

Z. Arzoumanian, A. Brazier, S. Burke-Spolaor +36

The North American Nanohertz Observatory for Gravitational Waves (NANOGrav) project currently observes 43 pulsars using the Green Bank and Arecibo radio telescopes. In this work we…

astro-ph.GA2012

A compact steep spectrum radio source in NGC1977

D. Anish Roshi, Scott M. Ransom

A compact steep spectrum radio source (J0535-0452) is located in the sky coincident with a bright optical rim in the HII region NGC1977. J0535-0452 is observed to be mas…

astro-ph.GA2012★ 48 cited

High resolution reddening map in the direction of the stellar system Terzan 5

Davide Massari, Alessio Mucciarelli, Emanuele Dalessandro +7

We have used optical images acquired with the Hubble Space Telescope to construct the first high-resolution extinction map in the direction of Terzan 5, a peculiar stellar system i…

astro-ph.GA2012★ 21 cited

Correlation of Chandra photons with the radio giant pulses from the Crab pulsar

A. V. Bilous, M. A. McLaughlin, V. I. Kondratiev +1

No apparent correlation was found between giant pulses (GPs) and X-ray photons from the Crab pulsar during 5.4 hours of simultaneous observations with the Green Bank Telescope at 1…

astro-ph.GA2012★ 20 cited

The Double Pulsar Eclipses I: Phenomenology and Multi-frequency Analysis

R. P. Breton, V. M. Kaspi, M. A. McLaughlin +7

The double pulsar PSR J0737-3039A/B displays short, 30 s eclipses that arise around conjunction when the radio waves emitted by pulsar A are absorbed as they propagate through the…

astro-ph.GA2011★ 128 cited

PSR J1841-0500: a radio pulsar that mostly is not there

F. Camilo, S. M. Ransom, S. Chatterjee +2

In a search for radio pulsations from the magnetar 1E 1841-045, we have discovered the unrelated pulsar J1841-0500, with rotation period P=0.9 s and characteristic age 0.4 Myr. One…

astro-ph.GA2011★ 28 cited

PSR J2030+3641: radio discovery and gamma-ray study of a middle-aged pulsar in the now identified Fermi-LAT source 1FGL J2030.0+3641

F. Camilo, M. Kerr, P. S. Ray +14

In a radio search with the Green Bank Telescope of three unidentified low Galactic latitude Fermi-LAT sources, we have discovered the middle-aged pulsar J2030+3641, associated with…

astro-ph.GA2011★ 82 cited

Fermi Detection of a Luminous Gamma-ray Pulsar in a Globular Cluster

The Fermi LAT Collaboration

We report the Fermi Large Area Telescope detection of gamma-ray (>100 megaelectronvolts) pulsations from pulsar J1823-3021A in the globular cluster NGC 6624 with high significance…

astro-ph.GA2011★ 31 cited

Arecibo PALFA Survey and Einstein@Home: Binary Pulsar Discovery by Volunteer Computing

B. Knispel, P. Lazarus, B. Allen +35

We report the discovery of the 20.7 ms binary pulsar J1952+2630, made using the distributed computing project Einstein@Home in Pulsar ALFA survey observations with the Arecibo tele…

astro-ph.GA2011★ 25 cited

Correlation of Fermi photons with high-frequency radio giant pulses from the Crab pulsar

A. V. Bilous, V. I. Kondratiev, M. A. McLaughlin +4

To constrain the giant pulse (GP) emission mechanism and test the model of Lyutikov (2007) for GP emission, we have carried out a campaign of simultaneous observations of the Crab…

astro-ph.GA2011

Non-Recycled Pulsars in Globular Clusters

Ryan S. Lynch, Jason R. Boyles, Duncan R. Lorimer +3

We place limits on the population of non-recycled pulsars originating in globular clusters through Monte Carlo simulations and frequentist statistical techniques. We set upper limi…

astro-ph.GA2011★ 6 cited

A New Pulsar in Green Bank Telescope Searches of Ten Globular Clusters

Ryan S. Lynch, Scott M. Ransom

We report the results of pulsar searches in ten globular clusters using the Robert C. Byrd Green Bank Telescope. One new binary millisecond pulsar has been discovered in NGC 5986 w…

astro-ph.GA2010★ 314 cited

On the nature and evolution of the unique binary pulsar J1903+0327

P. C. C. Freire, C. G. Bassa, N. Wex +16

(abridged) PSR J1903+0327, a millisecond pulsar in an eccentric (e = 0.44) 95-day orbit with a (~ 1Msun) companion poses a challenge to our understanding of stellar evolution in bi…

astro-ph.GA2010★ 69 cited

Pulsar Discovery by Global Volunteer Computing

B. Knispel, B. Allen, J. M. Cordes +37

Einstein@Home aggregates the computer power of hundreds of thousands of volunteers from 192 countries to "mine" large data sets. It has now found a 40.8 Hz isolated pulsar in radio…