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Optical variability patterns of radio-quiet and radio-loud quasars

Published online by Cambridge University Press:  23 June 2017

P. Marziani Open the ORCID record for P. Marziani [Opens in a new window] ,
E. Bon ,
A. Grieco ,
N. Bon ,
D. Dultzin ,
A. Del Olmo  and
M. D'Onofrio
P. Marziani
Affiliation:
INAF, Osservatorio Astronomico di Padova, Italy email: paola.marziani@oapd.inaf.it
E. Bon
Affiliation:
Belgrade Observatory, Serbia
A. Grieco
Affiliation:
Via Carpane 78, Vigonza, Italy
N. Bon
Affiliation:
Belgrade Observatory, Serbia
D. Dultzin
Affiliation:
Instituto de Astronomía, UNAM, Mexico
A. Del Olmo
Affiliation:
IAA (CSIC), Granada, Spain
M. D'Onofrio
Affiliation:
Università di Padova, Italy
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Abstract

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We analyzed the light curves (LCs) of several radio-quiet and radio-loud quasars belonging to the same parameter space volume in the 4D Eigenvector 1 (4DE1) quasar sequence, using data from the Catalina Real-time Transient Survey (CRTS). We report preliminary results on detected variability pattern, and discuss possible cases of periodic variability.

Keywords

quasars: generalblack hole physicsaccretionaccretion disksgalaxies: jets
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 243 - 244
Copyright
Copyright © International Astronomical Union 2017 

References

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