Abstract.
We monitored the BL Lac object S5 0716+714 in five intermediate optical passbands from 2004 September to 2011 April. The object was active most of the time and intra-day variability was frequently observed. The total variation amplitude tended to decrease with decreasing frequency. Strong bluer-when-brighter chromatism was observed on both long and short timescales.
Similar content being viewed by others
References
Chandra, S., Baliyan, K. S., Ganesh, S., Joshi, U. C. 2011, ApJ, 731, 118.
Dai, Y. et al. 2012, ApJS, 204, 22.
de Diego, J. A. 2010, AJ, 139, 1269.
Fan, J. et al. 2011, RAA, 11, 1311.
Ghisellini, G. et al. 1997, A&A, 327, 61.
Gu, M. et al. 2006, A&A, 450, 39.
Gu, M., Ai, Y. 2011, A&A, 528, 95.
Liu, X. et al. 2012, A&A, 543, 78.
Montagni, F. et al. 2006, A&A, 451, 435.
Nesci, R., Massaro, E., Montagni, F. 2002, PASA, 19, 143.
Nilsson, K. et al. 2008, A&A, 487, L29.
Quirrenbach, A. et al. 1991, ApJ, 372, 71.
Raiteri, C. M. et al. 2003, A&A, 402, 151.
Sasada, M. et al. 2008, PASJ, 60, L37.
Villata, M. et al. 2000, A&A, 363, 108.
Wagner, S., Witzel, A. 1995, ARAA, 33, 163.
Wagner, S. J. et al. 1996, AJ, 111, 2187.
Wu, J. et al. 2005, AJ, 129, 1818.
Wu, J. et al. 2007, AJ, 133, 1599.
Zhang, B. et al. 2012, MNRAS, 421, 3111.
Zhou, X. et al. 2003, A&A, 397, 361.
Acknowledgements
We thank the anonymous referee for his/her comments and suggestions. This work is supported by the Chinese National Natural Science Foundation (Grant No. 11273006) and the National Basic Research Programme of China 973 Program 2013CB834900.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Wu, J., Dai, Y., Zhou, X. et al. Seven-Year Multi-Colour Optical Monitoring of BL Lacertae Object S5 0716+714. J Astrophys Astron 35, 315–319 (2014). https://doi.org/10.1007/s12036-014-9220-1
Published:
Issue Date:
DOI: https://doi.org/10.1007/s12036-014-9220-1