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S. J. Chamberlin

Researcher at Pennsylvania State University

Publications -  151
Citations -  54314

S. J. Chamberlin is an academic researcher from Pennsylvania State University. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 72, co-authored 151 publications receiving 45442 citations. Previous affiliations of S. J. Chamberlin include University of Wisconsin–Milwaukee.

Papers
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Properties of the binary neutron star merger GW170817

B. P. Abbott, +1146 more
TL;DR: In this article, the authors improved initial estimates of the binary's properties, including component masses, spins, and tidal parameters, using the known source location, improved modeling, and recalibrated Virgo data.
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Tests of general relativity with the binary black hole signals from the LIGO-Virgo catalog GWTC-1

B. P. Abbott, +1141 more
- 20 Nov 2019 - 
TL;DR: In this paper, the authors present four tests of the consistency of the data with binary black hole gravitational waveforms predicted by general relativity, including the best-fit waveform from the data and the consistency with detector noise.
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The NANOGrav 11-year Data Set: High-precision Timing of 45 Millisecond Pulsars

Zaven Arzoumanian, +55 more
TL;DR: In this article, the authors presented high-precision timing data over time spans of up to 11 years for 45 millisecond pulsars observed as part of the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) project, aimed at detecting and characterizing low-frequency gravitational waves.
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Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo

B. P. Abbott, +1218 more
TL;DR: In this paper, the mass, spin, and redshift distributions of binary black hole (BBH) mergers with LIGO and Advanced Virgo observations were analyzed using phenomenological population models.
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The NANOGrav 11-year Data Set: Pulsar-timing Constraints On The Stochastic Gravitational-wave Background

Zaven Arzoumanian, +60 more
TL;DR: In this paper, an isotropic stochastic GWB in the newly released 11-year data set from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) was searched for and the first pulsar-timing array (PTA) constraints that are robust against SSE errors were obtained.