# Radio and optical intra-day variability observations of five blazars

**Authors:** X. Liu, P.P. Yang, J. Liu, B.R. Liu, S.M. Hu, O.M. Kurtanidze, S., Zola, A. Kraus, T.P. Krichbaum, R.Z. Su, K. Gazeas, K. Sadakane, K. Nilson,, D.E. Reichart, M. Kidger, K. Matsumoto, S. Okano, M. Siwak, J.R. Webb, T., Pursimo, F. Garcia, R. Naves Nogues, A. Erdem, F. Alicavus, T. Balonek, S.G., Jorstad

arXiv: 1705.00124 · 2017-05-04

## TL;DR

This study presents simultaneous radio and optical intra-day variability observations of five blazars, revealing significant variability with some quasi-periodic behavior and weak correlations between bands, highlighting different underlying mechanisms.

## Contribution

First simultaneous multi-band intra-day variability observations of five blazars, analyzing variability amplitudes, timescales, and potential periodicity across radio and optical bands.

## Key findings

- Blazars show significant intra-day variability in radio and optical bands.
- B0925+504 exhibits strong quasi-periodic radio variability.
- Weak correlation observed between radio and optical variability in some sources.

## Abstract

We carried out a pilot campaign of radio and optical band intra-day variability (IDV) observations of five blazars (3C66A, S5 0716+714, OJ287, B0925+504, and BL Lacertae) on December 18--21, 2015 by using the radio telescope in Effelsberg (Germany) and several optical telescopes in Asia, Europe, and America. After calibration, the light curves from both 5 GHz radio band and the optical R band were obtained, although the data were not smoothly sampled over the sampling period of about four days. We tentatively analyse the amplitudes and time scales of the variabilities, and any possible periodicity. The blazars vary significantly in the radio (except 3C66A and BL Lacertae with only marginal variations) and optical bands on intra- and inter-day time scales, and the source B0925+504 exhibits a strong quasi-periodic radio variability. No significant correlation between the radio- and optical-band variability appears in the five sources, which we attribute to the radio IDV being dominated by interstellar scintillation whereas the optical variability comes from the source itself. However, the radio- and optical-band variations appear to be weakly correlated in some sources and should be investigated based on well-sampled data from future observations.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1705.00124/full.md

## References

64 references — full list in the complete paper: https://tomesphere.com/paper/1705.00124/full.md

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Source: https://tomesphere.com/paper/1705.00124