A Correlation of Spectral Lag Evolution with Prompt Optical Emission in GRBs?
Michael Stamatikos, Tilan N. Ukwatta, Takanori Sakamoto, Kalvir S., Dhuga

TL;DR
This study reveals a correlation between spectral lag evolution and prompt optical emission in GRB 080319B, suggesting a coupled radiation mechanism and source region, with implications for understanding shock dynamics in gamma-ray bursts.
Contribution
Introduces a new cross-correlation function methodology to analyze spectral lag evolution and links it to prompt optical emission in GRBs, providing observational evidence of their connection.
Findings
Anti-correlation between gamma-ray and optical spectral lags.
Optical emission coincides with specific spectral lag behaviors.
Spectral lag dynamics relate to shock evolution in GRBs.
Abstract
We report on observations of correlated behavior between the prompt gamma-ray and optical emission from GRB 080319B, which (i) strongly suggest that they occurred within the same astrophysical source region and (ii) indicate that their respective radiation mechanisms were most likely dynamically coupled. Our preliminary results, based upon a new cross-correlation function (CCF) methodology for determining the time-resolved spectral lag, are summarized as follows. First, the evolution in the arrival offset of prompt gamma-ray photon counts between Swift-BAT 15-25 keV and 50-100 keV energy bands (intrinsic gamma-ray spectral lag) appears to be anti-correlated with the arrival offset between prompt 15-350 keV gamma-rays and the optical emission observed by TORTORA (extrinsic optical/gamma-ray spectral lag), thus effectively partitioning the burst into two main episodes at ~T+28+/-2 sec.…
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