Swift and NuSTAR observations of GW170817: Detection of a blue kilonova
University of Leicester · National Centre for Earth Observation · +26 more institutions
Abstract
GROWTH observations of GW170817 The gravitational wave event GW170817 was caused by the merger of two neutron stars (see the Introduction by Smith). In three papers, teams associated with the GROWTH (Global Relay of Observatories Watching Transients Happen) project present their observations of the event at wavelengths from x-rays to radio waves. Evans et al. used space telescopes to detect GW170817 in the ultraviolet and place limits on its x-ray flux, showing that the merger generated a hot explosion known as a blue kilonova. Hallinan et al. describe radio emissions generated as the explosion slammed into the surrounding gas within the host galaxy. Kasliwal et al. present additional observations in the…
Citation impact
- FWCI
- 51.10
- Percentile
- 100%
- References
- 80
Authors
59- PAP. A. EvansCorresponding
University of Leicester, National Centre for Earth Observation
- SBS. B. Cenko
Goddard Space Flight Center, Joint Space Science Institute, Deleted Institution, University of Maryland, College Park
- JAJ. A. Kennea
Pennsylvania State University
- SWS. W. K. Emery
University College London
- NPN. P. M. Kuin
University College London
Topics & keywords
- Kilonova
- Orbital plane
- Ejecta
- Telescope
- Gravitational wave
- Neutron star
- Ultraviolet
- Collimated light
Funding
- UDU.S. Department of EnergyAwards: DE-AC52-06NA25396, AC52-06NA25396
- NNNational Nuclear Security AdministrationAward: DE-AC52-06NA25396
- SAScience and Technology Facilities CouncilAwards: ST/L000733/1, ST/P000495/1, ST/N000757/1, ST/N000811/1, 1579029, ST/H001972/1
- LALos Alamos National LaboratoryAwards: AC52-06NA25396, DE-AC52-06NA25396