JINA - Segue Virtual Journal,
20 October 2017
Volume 12, Issue 42 (88 Articles)
- # 4 - A kilonova as the electromagnetic counterpart to a gravitational-wave source. (arXiv:1710.05841v1 [astro-ph.HE])
- S. J. Smartt, T.-W. Chen, A. Jerkstrand, M. Coughlin, E. Kankare, S. A. Sim, M. Fraser, C. Inserra, K. Maguire, K. C. Chambers, M. E. Huber, T. Kruhler, G. Leloudas, M. Magee, L. J. Shingles, K. W. Smith, D. R. Young, J. Tonry, R. Kotak, A. Gal-Yam, J. D. Lyman, D. S. Homan, C. Agliozzo, J. P. Anderson, C. R. Angus C. Ashall, C. Barbarino, F. E. Bauer, M. Berton, M. T. Botticella, M. Bulla, J. Bulger, G. Cannizzaro, Z. Cano, R. Cartier, A. Cikota, P. Clark, A. De Cia, M. Della Valle, L. Denneau, M. Dennefeld, L. Dessart, G. Dimitriadis, N. Elias-Rosa, R. E. Firth, H. Flewelling, A. Flors, A. Franckowiak, C. Frohmaier, L. Galbany, S. Gonzalez-Gaitan, J. Greiner, M. Gromadzki, A. Nicuesa Guelbenzu, C. P. Gutierrez, A. Hamanowicz, L. Hanlon, J. Harmanen, K. E. Heintz, A. Heinze, M.-S. Hernandez, et al. (61 additional authors not shown)
- http://arxiv.org/abs/1710.05841
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
