We present the light curve data of a remarkable blazer 3C 454.3 (z=0.859) in optical, X-ray, and gamma-ray bands. Since January 2008, we have been monitoring this object using the 50 cm MITSuME, a optical telescope, and detected several flares including extraordinary and simultaneous flares in the γ-ray and optical bands in November 2010. Additionally, the Monitor of All-sky Image (MAXI) has been observing 3C 454.3 continuously since August 2009. Using these data and gamma-ray flux observed with Fermi-LAT, we discuss features and correlations of flux variations between the energy bands.
@article{arxiv.1502.03610,
title = {A Correlation Between Optical, X-ray, and Gamma-ray Variations in Blazar 3C 454.3},
author = {Yutaro Tachibana and Nobuyuki Kawai and Sean Pike},
journal= {arXiv preprint arXiv:1502.03610},
year = {2019}
}