X-ray/UV/optical variability of NGC 4593 with Swift: reprocessing of X-rays by an extended reprocessor Article

McHardy, IM, Connolly, SD, Horne, K et al. (2018). X-ray/UV/optical variability of NGC 4593 with Swift: reprocessing of X-rays by an extended reprocessor . MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 480(3), 2881-2897. 10.1093/mnras/sty1983

Open Access Industry Collaboration International Collaboration

cited authors

  • McHardy, IM; Connolly, SD; Horne, K; Cackett, EM; Gelbord, J; Peterson, BM; Pahari, M; Gehrels, N; Goad, M; Lira, P; Arevalo, P; Baldi, RD; Brandt, N; Breedt, E; Chand, H; Dewangan, G; Done, C; Elvis, M; Emmanoulopoulos, D; Fausnaugh, MM; Kaspi, S; Kochanek, CS; Korista, K; Papadakis, IE; Rao, AR; Uttley, P; Vestergaard, M; Ward, MJ

authors

publication date

  • November 1, 2018

keywords

  • ACCRETION DISCS
  • ACTIVE GALACTIC NUCLEI
  • Astronomy & Astrophysics
  • BLACK-HOLE MASS
  • CONTINUUM EMISSION
  • LIGHT CURVES
  • OPTICAL VARIABILITY
  • Physical Sciences
  • RAY/ULTRAVIOLET/OPTICAL VARIABILITY
  • SEYFERT-GALAXIES
  • SPECTRAL VARIABILITY
  • Science & Technology
  • X-rays: galaxies
  • XMM-NEWTON
  • galaxies: Seyfert
  • galaxies: active
  • galaxies: individual: NGC 4593
  • ultraviolet: galaxies

Digital Object Identifier (DOI)

publisher

  • OXFORD UNIV PRESS

start page

  • 2881

end page

  • 2897

volume

  • 480

issue

  • 3