Published May 18, 2022
| Version 1.0.0
Dataset
Open
NMMA: A nuclear-physics and multi-messenger astrophysics framework to analyze binary neutron star mergers
Authors/Creators
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Pang, Peter Tsun Ho1
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Dietrich, Tim2
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Coughlin, Michael3
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Bulla, Mattia4
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Tews, Ingo5
- Almualla, Mouza6
- Barna, Tyler3
- Kiendrebeogo, Weizmann7
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Kunert, Nina2
- Mansingh, Gargi3
- Reed, Brandon3
- Sravan, Niharika8
- Toivonen, Andrew3
- Antier, Sarah9
- VandenBerg, Robert O.3
- Heinzel, Jack10
- Nedora, Vsevolod11
- Salehi, Pouyan2
- Sharma, Ritwik12
- Somasundaram, Rahul13
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Van Den Broeck, Chris1
- 1. Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University
- 2. Institut für Physik und Astronomie, Universität Potsdam
- 3. School of Physics and Astronomy, University of Minnesota
- 4. The Oskar Klein Centre, Department of Astronomy, Stockholm University
- 5. Theoretical Division, Los Alamos National Laboratory
- 6. Department of Physics, American University of Sharjah
- 7. Laboratoire de Physique et de Chimie de l'Environnement, Universit ́e Joseph KI-ZERBO
- 8. Division of Physics, Mathematics, and Astronomy, California Institute of Technology
- 9. Artemis, Universit ́e C ˆote d'Azur, Observatoire C ˆote d'Azur, CNRS
- 10. Department of Physics, Massachusetts Institute of Technology
- 11. Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
- 12. Department of Physics, Deshbandhu College, University of Delhi
- 13. Univ Lyon, Univ Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon
Description
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
Files
Files
(70.8 MB)
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md5:e128443b2b0a7e8e57e7a4f52c544b7a
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70.8 MB | Download |