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