Bhatta G.; Goyal A.; Ostrowski M.; Stawarz; Akitaya H.; Arkharov A.; Bachev R.; Benítez E.; Borman G.; Carosati D.; Cason A.; Damljanovic G.; Dhalla S.; Frasca A.; Hu S.; Itoh R.; Jorstad S.; Jableka D.; Kawabata K.; Klimanov S.; Kurtanidze O.; Larionov V.; Laurence D.; Leto G.; Markowitz A.; Marscher A.; Moody J.; Moritani Y.; Ohlert J.; Di Paola A.; Raiteri C.; Rizzi N.; Sadun A.; Sasada M.; Sergeev S.; Strigachev A.; Takaki K.; Troitsky I.; Ui T.; Villata M.; Vince O.; Webb J.; Yoshida M.; Zola S.; Hiriart D.
(2015)
© 2015. The American Astronomical Society. All rights reserved. The occurrence of low-amplitude flux variations in blazars on hourly timescales, commonly known as microvariability, is still a widely debated subject in ...