Multi-wavelength Temporal Variability of the Blazar 3C 454.3 during 2014 Activity Phase
Pankaj Kushwaha (1, 2), Alok C. Gupta (3,4), Ranjeev Misra (1), K. P., Singh (5) ((1) IUCAA, Pune, India (2) IAG-USP, Brazil (3) ARIES, Nainital,, India (4) SAO, Shanghai, China (5) TIFR, Mumbai, India)

TL;DR
This study analyzes the multi-wavelength variability of blazar 3C 454.3 during 2014, revealing changes in emission lag times and supporting a magnetic field-related origin for its high-energy emissions.
Contribution
It provides the first detailed multi-band correlation analysis of 3C 454.3 during a high activity phase, highlighting variable lag patterns and consistent emission region conditions.
Findings
Gamma-ray lags vary from no lag to ~3 days behind IR/optical.
Emission region remains localized and similar across activity states.
X-ray and gamma-ray emissions are likely inverse Comptonized IR/optical photons.
Abstract
We present a multi-wavelength temporal analysis of the blazar 3C 454.3 during the high -ray active period from May-December, 2014. Except for X-rays, the period is well sampled at near-infrared (NIR)-optical by the \emph{SMARTS} facility and the source is detected continuously on daily timescale in the \emph{Fermi}-LAT -ray band. The source exhibits diverse levels of variability with many flaring/active states in the continuously sampled -ray light curve which are also reflected in the NIR-optical light curves and the sparsely sampled X-ray light curve by the \emph{Swift}-XRT. Multi-band correlation analysis of this continuous segment during different activity periods shows a change of state from no lags between IR and -ray, optical and -ray, and IR and optical to a state where -ray lags the IR/optical by 3 days. The results are…
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