Search Results - "Lommen, A. N."
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Arecibo timing and single-pulse observations of 17 pulsars
Published in Monthly notices of the Royal Astronomical Society (01-11-2005)“…We report on timing and single-pulse observations of 17 pulsars discovered at the Arecibo Observatory. The highlights of our sample are the recycled pulsars…”
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Using Pulsars to Detect Massive Black Hole Binaries via Gravitational Radiation: Sagittarius A and Nearby Galaxies
Published in The Astrophysical journal (20-11-2001)Get full text
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LIMITS ON THE STOCHASTIC GRAVITATIONAL WAVE BACKGROUND FROM THE NORTH AMERICAN NANOHERTZ OBSERVATORY FOR GRAVITATIONAL WAVES
Published in The Astrophysical journal (10-01-2013)“…We present an analysis of high-precision pulsar timing data taken as part of the North American Nanohertz Observatory for Gravitational Waves (NANOGrav)…”
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GRAVITATIONAL WAVES FROM INDIVIDUAL SUPERMASSIVE BLACK HOLE BINARIES IN CIRCULAR ORBITS: LIMITS FROM THE NORTH AMERICAN NANOHERTZ OBSERVATORY FOR GRAVITATIONAL WAVES
Published in The Astrophysical journal (20-10-2014)“…We perform a search for continuous gravitational waves from individual supermassive black hole binaries using robust frequentist and Bayesian techniques. We…”
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PSR J0609+2130: a disrupted binary pulsar?
Published in Monthly notices of the Royal Astronomical Society (11-01-2004)“…We report the discovery and initial timing observations of a 55.7-ms pulsar, J0609+2130, found during a 430-MHz drift-scan survey with the Arecibo radio…”
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The NANOGrav 11 yr Data Set: Evolution of Gravitational-wave Background Statistics
Published in The Astrophysical journal (20-02-2020)“…An ensemble of inspiraling supermassive black hole binaries should produce a stochastic background of very low frequency gravitational waves. This stochastic…”
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PSR J1740+1000: A Young Pulsar Well Out of the Galactic Plane
Published in The Astrophysical journal (01-01-2002)Get full text
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Masses, Parallax, and Relativistic Timing of the PSR J1713+0747 Binary System
Published in The Astrophysical journal (10-02-2005)“…We report on 12 years of observations of PSR J1713+0747, a pulsar in a 68 day orbit with a white dwarf. Pulse times of arrival were measured with uncertainties…”
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The Parallax and Proper Motion of PSR J0030+0451
Published in The Astrophysical journal (10-05-2006)“…We report the parallax and proper motion of millisecond pulsar J0030+0451, one of 13 known isolated millisecond pulsars in the disk of the Galaxy. We obtained…”
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THE NANOGRAV NINE-YEAR DATA SET: LIMITS ON THE ISOTROPIC STOCHASTIC GRAVITATIONAL WAVE BACKGROUND
Published in The Astrophysical journal (10-04-2016)“…ABSTRACT We compute upper limits on the nanohertz-frequency isotropic stochastic gravitational wave background (GWB) using the 9 year data set from the North…”
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NANOGrav CONSTRAINTS ON GRAVITATIONAL WAVE BURSTS WITH MEMORY
Published in The Astrophysical journal (10-09-2015)“…ABSTRACT Among efforts to detect gravitational radiation, pulsar timing arrays are uniquely poised to detect "memory" signatures, permanent perturbations in…”
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Studying the Solar system with the International Pulsar Timing Array
Published in Monthly notices of the Royal Astronomical Society (01-12-2018)“…Pulsar-timing analyses are sensitive to errors in the Solar-system ephemerides (SSEs) that timing models utilize to estimate the location of the Solar-system…”
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The NANOGrav 11-Year Data Set: Evolution of Gravitational Wave Background Statistics
Published 20-09-2019“…An ensemble of inspiraling supermassive black hole binaries should produce a stochastic background of very low frequency gravitational waves. This stochastic…”
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The NANOGrav 11-year Data Set: Pulsar-timing Constraints On The Stochastic Gravitational-wave Background
Published 07-06-2018“…The Astrophysical Journal, Volume 859, Number 1, 2018 We search for an isotropic stochastic gravitational-wave background (GWB) in the newly released $11$-year…”
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Arecibo Pulsar Survey Using ALFA. II. The Young, Highly Relativistic Binary Pulsar J1906+0746
Published in The Astrophysical journal (20-03-2006)“…We report the discovery of PSR J1906+0746, a young 144 ms pulsar in a highly relativistic 3.98 hr orbit with an eccentricity of 0.085 and expected…”
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The NANOGrav Nine-year Data Set: Observations, Arrival Time Measurements, and Analysis of 37 Millisecond Pulsars
Published 05-01-2016“…The Astrophysical Journal, Volume 813, Issue 1, article id. 65, 31 pp. (2015) We present high-precision timing observations spanning up to nine years for 37…”
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NANOGrav Constraints on Gravitational Wave Bursts with Memory
Published 21-01-2015“…Among efforts to detect gravitational radiation, pulsar timing arrays are uniquely poised to detect "memory" signatures, permanent perturbations in spacetime…”
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NANOGrav Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries in Circular Orbits
Published 20-05-2014“…The North American Nanohertz Observatory for Gravitational Waves (NANOGrav) project currently observes 43 pulsars using the Green Bank and Arecibo radio…”
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Limits on the Stochastic Gravitational Wave Background from the North American Nanohertz Observatory for Gravitational Waves
Published 31-01-2012“…We present an analysis of high-precision pulsar timing data taken as part of the North American Nanohertz Observatory for Gravitational waves (NANOGrav)…”
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Measuring the mass of solar system planets using pulsar timing
Published 21-08-2010“…High-precision pulsar timing relies on a solar-system ephemeris in order to convert times of arrival (TOAs) of pulses measured at an observatory to the solar…”
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