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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2022
License: CC BY
Data sources: ZENODO
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Claim

NMMA: A nuclear-physics and multi-messenger astrophysics framework to analyze binary neutron star mergers

Research datakeyboard_double_arrow_right Dataset 18 May 2022 English Publisher:ZenodoFunded by:NSF | Extending the Reach of Gr..., NSF | HDR Institute: Accelerate..., EC | SMArt +2 projects
Authors: Pang, Peter Tsun Ho; Dietrich, Tim; Coughlin, Michael; Bulla, Mattia; Tews, Ingo; Almualla, Mouza; Barna, Tyler; +14 Authors

doi: 10.5281/zenodo.6551052 , 10.5281/zenodo.6551053

NMMA: A nuclear-physics and multi-messenger astrophysics framework to analyze binary neutron star mergers

Abstract

Data release associated with the preprint "NMMA: A nuclear-physics and multi-messenger astrophysics framework to analyze binary neutron star mergers" Data includes: EOS files: 5000 eos files with radius (km), mass (Msun), and tidal deformability as columns stored under eos/eos_data prior probabilities for the EOSs are stored in eos/eos_prior_probability.dat Posterior samples: Posterior samples based on the analysis of GW170817 and AT2017gfo stored in posterior_samples/GW170817-AT2017gfo_posterior_samples.dat Posterior samples based on the analysis of GW170817, AT2017gfo, and the afterglow of GRB170817A are stored in posterior_samples/GW170817-AT2017gfo-GRB170817A_afterglow_posterior_samples.dat

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Keywords

neutron star core, gravitational waves, nuclear physics, stellar mergers, gamma-ray-burst, neutron stars, kilonova

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
views
OpenAIRE UsageCountsViews provided by UsageCounts
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