Abstract
We compiled the radio, optical and X-ray data for SDSS sample, and presented broad band spectral index. The broad band energy distribution reveals that FSRQs and LBLs objects have similar spectral properties. However, HBLs have a separate distinct property. Even so, a unified scheme was also revealed from colour–colour diagram.
Similar content being viewed by others
References
Antón S. and Browne I. W. A. 2005, Mon. Not. R. Astron. Soc., 356, 225.
Chen Z. Y., Gu M. F., and Cao X. W. 2009, Mon. Not. R. Astron. Soc., 397, 1713.
Fossati G., Maraschi L., et al. 1998, Mon. Not. R. Astron. Soc., 299, 433.
Li H. Z., Xie G. Z., Yi T. F., et al. 2010, Astrophys. J., 709, 1407.
Plotkin Ri. M., Anderson S. F., Hall P. B., et al. 2008, Astron. J., 135, 2453.
Xie G. Z., Ding S. X., Dai H., et al. 2003, Int. J. Mod. Phys. D., 12, 781.
Acknowledgements
This work is supported by the National Natural Science Foundation of China (No. 10878013), the Natural Science Foundation of Yunnan Province (2013FB063, 2011FZ081, 2012FD055), the Programme for Innovative Research Team (in Science and Technology) in the University of Yunnan Province (IRTSTYN), and Science Research Foundation of Yunnan Education Department of China (2012Y316).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Li, H.Z., Chen, L.E. Spectral Energy Distributions of SDSS Blazars. J Astrophys Astron 35, 387–389 (2014). https://doi.org/10.1007/s12036-014-9237-5
Published:
Issue Date:
DOI: https://doi.org/10.1007/s12036-014-9237-5