no code implementations • 9 Dec 2020 • S. E. M. de Haas, T. D. Russell, N. Degenaar, S. Markoff, A. J. Tetarenko, B. E. Tetarenko, J. van den Eijnden, J. C. A. Miller-Jones, A. S. Parikh, R. M. Plotkin, G. R. Sivakoff
During this outburst, GX 339-4 showed no atypical X-ray behaviour that may act as a indicator for an outburst remaining within the hard state.
High Energy Astrophysical Phenomena
1 code implementation • 6 Oct 2014 • J. J. Ruan, S. F. Anderson, R. M. Plotkin, W. N. Brandt, T. H. Burnett, A. D. Myers, D. P. Schneider
Blazars are classically divided into the BL Lac (BLL) and Flat-Spectrum Radio Quasar (FSRQ) subclasses, corresponding to radiatively inefficient and efficient accretion regimes, respectively, largely based on the equivalent width (EW) of their optical broad emission lines (BEL).
High Energy Astrophysical Phenomena
