Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source
University of California, Santa Cruz · Carnegie Institution for Science · +10 more institutions
Abstract
Photons from a gravitational wave event Two neutron stars merging together generate a gravitational wave signal and have also been predicted to emit electromagnetic radiation. When the gravitational wave event GW170817 was detected, astronomers rushed to search for the source using conventional telescopes (see the Introduction by Smith). Coulter et al. describe how the One-Meter Two-Hemispheres (1M2H) collaboration was the first to locate the electromagnetic source. Drout et al. present the 1M2H measurements of its optical and infrared brightness, and Shappee et al. report their spectroscopy of the event, which is unlike previously detected astronomical transient sources. Kilpatrick et al. show how these…
Citation impact
- FWCI
- 102.02
- Percentile
- 100%
- References
- 44
Authors
17- DAD. A. CoulterCorresponding
University of California, Santa Cruz
- RJR. J. Foley
University of California, Santa Cruz
- CDC. D. Kilpatrick
University of California, Santa Cruz
- MRM. R. Drout
Carnegie Institution for Science, Carnegie Observatories
- ALA. L. Piro
Carnegie Institution for Science, Carnegie Observatories
Topics & keywords
- Gravitational wave
- Neutron star
- Supernova
- LIGO
- Observatory
- Interferometry
- Galaxy
- Einstein Telescope