http://arxiv.org/abs/1809.04984
We collect long term $\gamma$-ray, optical and radio $15$ GHz light curves of the flat-spectrum radio quasar (FSRQ) object PMN J2345-1555. The correlation analyses between them are performed via the local cross-correlation function (LCCF). We found that all the optical $V$, $R$ band and the infrared $J$ band are correlated with the radio 15 GHz with significance larger than $3\sigma$, and the lag times are $-221.81^{+6.26}{-6.72}$, $-201.38^{+6.42}{-6.02}$ and $-192.27^{+8.26}{-7.37}$ days, respectively. However, the $\gamma$-ray is correlated with the radio at only $1.5 \sigma$ significance level, and the lag time is $-103.51^{+9.57}{-8.69}$ days. The lag times enable us to derive that the optical $V$ band and the $\gamma$-ray emitting regions are located at $5.47\pm0.31$ and $11.16\pm0.46$ parsec from the base of the jet, respectively. We present that time lags between different frequencies can be used as an alternative parameter to derive the core-shift measurement, and the magnetic field and particle density of jets can be derived by this method in a direct way. The variation of $R-J$ color index shows a bluer when brighter trend. We also found that a $3\sigma$ correlation between $\delta V-\delta R$ and the radio light curve, which indicates that opacity plays an important role in the variation. As hinted from radio images, we proposed that the upstream and downstream emission component contributes the bluer and redder spectral index, respectively. Such spatial dependent spectral index model is complementary for the shock in jet model, and provides a new mechanism to explain various spectral index behaviors of blazars in a unified way.
Y. Jiang, S. Hu, X. Chen, et. al.
Fri, 14 Sep 18
20/65
Comments: 10pages,12figures