Published January 6, 2023
| Version v2
Journal article
Open
Bayesian model selection for GRB 211211A through multi-wavelength analyses
Creators
- 1. Institute for Physics and Astronomy, University of Potsdam, D-14476 Potsdam, Germany
- 2. Artemis, Observatoire de la Côte d'Azur, Université Côte d'Azur, Boulevard de l'Observatoire, 06304 Nice, France
- 3. Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, Potsdam 14476, Germany
- 4. Department of Physics and Earth Science, University of Ferrara, via Saragat 1, I-44122 Ferrara, Italy
- 5. Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, The Netherlands
- 6. Cahill Center for Astrophysics, California Institute of Technology, Pasadena CA 91125, USA
- 7. School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
- 8. Theoretical Division, Los Alamos National Laboratory, Los Alamos, NM 87545, USA
- 9. Kavli Institute for Theoretical Physics, Kohn Hall, University of California, Santa Barbara, CA 93106, USA
- 10. IJCLab, Univ Paris-Saclay, CNRS/IN2P3, Orsay, France
- 11. Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA
- 12. Institute of Physics and Astronomy, Theoretical Astrophysics, University Potsdam, Haus 28, Karl-Liebknecht-Str. 24/25, 14476, Potsdam, Germany
Description
Posterior sample data obtained in the analysis of GRB 211211A for two different prior settings on the luminosity distance (narrow, wide), different models/model combinations (GRB-M, BNS-KN-Kasen, BNS-KN-Bulla, NSBH-KN-Bulla, SNCol, SN98bw) and two GRB jet types (gaussian, top-hat). AnBa2022_tf_GRB211211A.zip is the reduced model grid based on Barnes & Metzger, (2022), tailored to GRB 211211A, which can be used in the nuclear physics and multi-messenger astronomy framework NMMA, see also Pang, P. T. H., et al. (2022).
Files
AnBa2022_tf_GRB211211A.zip
Files
(107.0 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:e4929c7f2dc473531f96e52c9669462c
|
20.6 MB | Preview Download |
|
md5:4779a1b5d723ae56d5b55e04eb7b6b83
|
5.4 MB | Download |
|
md5:0b38b71b02819c8bf66e4f79537f9229
|
4.6 MB | Download |
|
md5:fb78d4a52922df2f0a72615d21416296
|
4.0 MB | Download |
|
md5:c752e633833d17cae13a61c910026795
|
3.7 MB | Download |
|
md5:a7e95ccda77f5e57f839b429f11d5b5e
|
3.2 MB | Download |
|
md5:cff62204c20a521bdccafb79a7eb4255
|
4.2 MB | Download |
|
md5:61a2b8841ec04e9e594eb5ab4d5fc868
|
3.3 MB | Download |
|
md5:d73a8789ccb467b6ec5f98f2b4ac9234
|
3.5 MB | Download |
|
md5:bfcd0146b74248f7c966188ff4d2b7b7
|
2.9 MB | Download |
|
md5:96f9f5a09b0bd6087384787846970529
|
2.7 MB | Download |
|
md5:d5ce50812057a663e21cfd2bc5a9441b
|
4.9 MB | Download |
|
md5:378e293172c9d09fd589efdb47b09063
|
4.2 MB | Download |
|
md5:92b300a2196d6dfd0451b9670d7e5db1
|
4.1 MB | Download |
|
md5:78a4c417dcb40f08de068d795fb56929
|
3.6 MB | Download |
|
md5:cd1d76b5c614137161ec57631110f476
|
3.0 MB | Download |
|
md5:8f0424a9295c9237f77a736d5df5400b
|
4.4 MB | Download |
|
md5:63426dbd5c0936306f196e9d33477b3d
|
3.8 MB | Download |
|
md5:487a189fbdecaa15d79fe3dc528f32ca
|
3.2 MB | Download |
|
md5:ffcfbe991eadb3def0db628bc20b8065
|
2.7 MB | Download |
|
md5:e747dbbecb20756b36505c10f507acbb
|
6.4 MB | Download |
|
md5:9756cfa9a0c48319f2bfe6b63fec3376
|
5.8 MB | Download |
|
md5:f884e776123c7a7703acc0ecbd10d753
|
2.6 MB | Download |
Additional details
References
- Barnes, J., & Metzger, B. D. 2022, The Astrophysical Journal Letters, 939, L29
- Pang, P. T. H., et al. 2022, arXiv:2205.08513