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Autor:
Trakhtenbrot, Benny, Arcavi, Iair, Ricci, Claudio, Tacchella, Sandro, Stern, Daniel, Netzer, Hagai, Jonker, Peter G., Horesh, Assaf, Mejía-Restrepo, Julián Esteban, Hosseinzadeh, Griffin, Hallefors, Valentina, Howell, D. Andrew, McCully, Curtis, Baloković, Mislav, Heida, Marianne, Kamraj, Nikita, Lansbury, George Benjamin, Wyrzykowski, Łukasz, Gromadzki, Mariusz, Hamanowicz, Aleksandra, Cenko, S. Bradley, Sand, David J., Hsiao, Eric Y., Phillips, Mark M., Diamond, Tiara R., Kara, Erin, Gendreau, Keith C., Arzoumanian, Zaven, Remillard, Ron
Accreting supermassive black holes (SMBHs) can exhibit variable emission across the electromagnetic spectrum and over a broad range of timescales. The variability of active galactic nuclei (AGNs) in the ultraviolet and optical is usually at the few t
Externí odkaz:
http://arxiv.org/abs/1901.03731