Follow Up of GW170817 and Its Electromagnetic Counterpart by Australian-Led Observing Programmes

Andreoni, Igor; Ackley, K.; Cooke, Jeff; Acharyya, Ayan; R. Allison, J.; E. Anderson, G.; C. B. Ashley, M.; Baade, D.; Bailes, M.; W. Bannister, K.; P. Beardsley, Adam; S. Bessell, M.; Bian, Fuyan; A. Bland, P.; Boër, M.; Booler, T.; Brandeker, A.; Brown, Ian; A. H. Buckley, D.; Chang, Seo-Won; M. Coward, D.; M. Crawford, Steven; Crisp, H.; Crosse, B.; Cucchiara, Antonino; Cupák, Martin; S. de Gois, J.; T. Deller, Adam; A. R. Devillepoix, Hadrien; Dobie, Dougal; Elmer, E.; Emrich, D.; Farah, Wael; J. Farrell, Tony; M. O. Franzen, T.; M. Gaensler, B.; K. Galloway, D.; Gendre, B.; W. Giblin, Timothy; Goobar, A.; Green, James; J. Hancock, P.; A. D. Hartig, Benjamin; J. Howell, E.; Horsley, L.; W. Hotan, A.; M. Howie, Robert; Hu, Lei; Hu, Yi-Ming; James, C.

doi:10.1017/pasa.2017.65

Public

Follow Up of GW170817 and Its Electromagnetic Counterpart by Australian-Led Observing Programmes

Shared by NobleBlocks on Jan 1, 2017 • 12:00 AM UTC

Authors:

Igor Andreoni

K. Ackley

Jeff Cooke

Abstract

Abstract The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era of multi-messenger astronomy. In this paper, we present follow-up observations of the gravitational wave event...

Subject

Physics

Neutron star

Astrophysics

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