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1 code implementation • 22 Mar 2021 • V. Ashley Villar, Miles Cranmer, Edo Berger, Gabriella Contardo, Shirley Ho, Griffin Hosseinzadeh, Joshua Yao-Yu Lin

There is a shortage of multi-wavelength and spectroscopic followup capabilities given the number of transient and variable astrophysical events discovered through wide-field, optical surveys such as the upcoming Vera C. Rubin Observatory.

no code implementations • 24 Dec 2020 • Plamen G. Krastev, Kiranjyot Gill, V. Ashley Villar, Edo Berger

One of the key challenges of real-time detection and parameter estimation of gravitational waves from compact binary mergers is the computational cost of conventional matched-filtering and Bayesian inference approaches.

Bayesian Inference Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology Nuclear Theory

no code implementations • 2 Nov 2020 • Hsin-Yu Chen, Philip S. Cowperthwaite, Brian D. Metzger, Edo Berger

With the larger BNS horizon distance in the Cosmic Explorer era, on-axis short gamma-ray bursts (SGRBs) and their afterglows (though accompanying only some of the GW-detected mergers) supplant kilonovae as the most promising counterparts for redshift identification.

Cosmology and Nongalactic Astrophysics

no code implementations • 3 Sep 2020 • Sebastian Gomez, Edo Berger, Peter K. Blanchard, Griffin Hosseinzadeh, Matt Nicholl, V. Ashley Villar, Yao Yin

This classifier can achieve a maximum purity of about 85\% (with 20\% completeness) when observing a selection of SLSN-I candidates.

High Energy Astrophysical Phenomena

2 code implementations • 23 Apr 2018 • Soumi De, Daniel Finstad, James M. Lattimer, Duncan A. Brown, Edo Berger, Christopher M. Biwer

We find that the tidal deformability and 90$\%$ credible interval is $\tilde{\Lambda}=310^{+679}_{-234}$ for a uniform component mass prior, $\tilde{\Lambda}=354^{+691}_{-245}$ for a component mass prior informed by radio observations of Galactic double neutron stars, and $\tilde{\Lambda}=334^{+669}_{-241}$ for a component mass prior informed by radio pulsars.

High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology

1 code implementation • 11 Apr 2018 • Daniel Finstad, Soumi De, Duncan A. Brown, Edo Berger, Christopher M. Biwer

The joint detection of gravitational waves (GWs) and electromagnetic (EM) radiation from the binary neutron star merger GW170817 ushered in a new era of multi-messenger astronomy.

High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology

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