1 code implementation • 11 Mar 2021 • Ryan-Rhys Griffiths, Jiachen Jiang, Douglas J. K. Buisson, Dan R. Wilkins, Luigi C. Gallo, Adam Ingram, Alpha A. Lee, Dirk Grupe, Erin Kara, Michael L. Parker, William Alston, Anthony Bourached, George Cann, Andrew Young, Stefanie Komossa
Such a reprocessing model would be characterised by lags between X-ray and optical/UV emission due to differences in light travel time.
Gaussian Processes High Energy Astrophysical Phenomena
no code implementations • 9 Mar 2021 • Jingyi Wang, Guglielmo Mastroserio, Erin Kara, Javier García, Adam Ingram, Riley Connors, Michiel van der Klis, Thomas Dauser, James Steiner, Douglas Buisson, Jeroen Homan, Matteo Lucchini, Andrew Fabian, Joe Bright, Rob Fender, Edward Cackett, Ron Remillard
We find the corona expansion (as probed by reverberation) precedes a radio flare by ~5 days, which may suggest that the hard-to-soft transition is marked by the corona expanding vertically and launching a jet knot that propagates along the jet stream at relativistic velocities.
High Energy Astrophysical Phenomena