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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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Journal ArticleDOI

Directional Limits on Persistent Gravitational Waves from Advanced LIGO’s First Observing Run

B. P. Abbott, +1018 more
TL;DR: Directed searches for narrowband gravitational waves from astrophysically interesting objects yield median frequency-dependent limits on strain amplitude at the most sensitive detector frequencies between 130-175 Hz, which represents a mean improvement of a factor of 2 across the band compared to previous searches of this kind.
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Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data

J. Aasi, +865 more
TL;DR: A search for the stochastic background with the latest data from the LIGO and Virgo detectors shows no evidence of a stochastically gravitational-wave signal, and the limits in these four bands are the lowest direct measurements to date on the stoChastic background.
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Model Comparison from LIGO-Virgo Data on GW170817's Binary Components and Consequences for the Merger Remnant

B. P. Abbott, +1280 more
TL;DR: In this paper, the authors perform Bayesian model selection on a wide range of theoretical predictions for the neutron star equation of state, and find that all scenarios from prompt collapse to long-lived or even stable remnants are possible.
Journal ArticleDOI

Improved Analysis of GW150914 Using a Fully Spin-Precessing Waveform Model

B. P. Abbott, +1001 more
- 21 Oct 2016 - 
TL;DR: In this paper, a 15-dimensional precessing-spin waveform model (precessing EOBNR) was developed within the EOB formalism for GW150914.
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Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914

B. P. Abbott, +719 more
- 28 Mar 2017 - 
TL;DR: In this article, the authors used a dedicated photon radiation pressure actuator, with cross-checks provided by optical and radio frequency references, to validate the model and characterize its uncertainty.