{"paper":{"title":"Gravity and Light: Combining Gravitational Wave and Electromagnetic Observations in the 2020s","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. Corsi, A. G. Riess, A. Horesh, A. I. MacFadyen, A. J. Levan, A. L. Piro, A. M. Beloborodov, A. Murguia-Berthier, A. Palmese, A. Rest, A. V. Filippenko, B. D. Metzger, B. Farr, B. Margalit, C. D. Kilpatrick, C. L. Fryer, C. L. Rodriguez, C. Pankow, C. Rojas-Bravo, D. A. Coulter, D. A. Frail, D. A. Howell, D. A. Perley, D. Hiramatsu, D. H. Shoemaker, D. Kasen, D. Lazzati, D. L. Coppejans, D. M. Siegel, D. O. Cook, D. O. Jones, D. Radice, E. C. Bellm, E. M. Rossi, E. O'Connor, E. Quataert, E. Ramirez-Ruiz, G. Baym, G. Dimitriadis, G. Hosseinzadeh, G. Narayan, G. Terreran, I. Andreoni, I. Arcavi, I. Mandel, J. Barnes, J. Cooke, J. C. Wheeler, J. H. Elias, J. Hjorth, J. McIver, J. M. Lattimer, J. M. O'Meara, J. P. Blakeslee, J. S. Brown, K. Auchettl, K. D. Alexander, K. Hotokezaka, K. Krisciunas, K. Maeda, K. Mooley, K. Nomoto, K. Paterson, K. Siellez, K. S. Mandel, L. Wang, M. Branchesi, M. Cantiello, M. Nicholl, M. R. Drout, M. R. Siebert, M. Ruiz, M. Soares-Santos, M. Tanaka, M. W. Coughlin, M. Zaldarriaga, M. Zevin, N. Blagorodnova, N. B. Suntzeff, N. Butler, N. R. Tanvir, N. Smith, P. K. G. Williams, P. R. Brady, P. S. Cowperthwaite, R. Chornock, R. Fernandez, R. J. Foley, R. Margutti, R. O'Shaughnessy, R. Perna, R. P. Kirshner, R. Surman, S. A. Webb, S. L. Shapiro, S. M. Couch, S. Nissanke, S. Reddy, S. Rosswog, S. Valenti, S. Woosley, T. A. Pritchard, T. Dietrich, T. Fragos, T. Hung, T. Moriya, V. A. Villar, V. Kalogera, V. Z. Golkhou, W. E. Kerzendorf, W. Fong, W. L. Freedman, Y.-C. Pan","submitted_at":"2019-03-11T19:20:36Z","abstract_excerpt":"As of today, we have directly detected exactly one source in both gravitational waves (GWs) and electromagnetic (EM) radiation, the binary neutron star merger GW170817, its associated gamma-ray burst GRB170817A, and the subsequent kilonova SSS17a/AT 2017gfo. Within ten years, we will detect hundreds of events, including new classes of events such as neutron-star-black-hole mergers, core-collapse supernovae, and almost certainly something completely unexpected. As we build this sample, we will explore exotic astrophysical topics ranging from nucleosynthesis, stellar evolution, general relativit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.04553","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}