Abstract:
We present a detailed prompt emission and early optical afterglow analysis of the two very-high-energy (VHE)
detected bursts GRB 201015A and GRB 201216C, and their comparison with a subset of similar bursts. Time resolved spectral analysis of multistructured GRB 201216C using the Bayesian binning algorithm revealed that
during the entire duration of the burst, the low-energy spectral index (αpt) remained below the limit of the
synchrotron line of death. However, statistically some of the bins supported the additional thermal component.
Additionally, the evolution of spectral parameters showed that both the peak energy (Ep) and αpt tracked the flux.
These results were further strengthened using the values of the physical parameters obtained by synchrotron
modeling of the data. Our earliest optical observations of both bursts using the F/Photometric Robotic
Atmospheric Monitor Observatorio del Roque de los Muchachos and Burst Observer and Optical Transient
Exploring System robotic telescopes displayed a smooth bump in their early optical light curves, consistent with
the onset of the afterglow due to synchrotron emission from an external forward shock. Using the observed optical
peak, we constrained the initial bulk Lorentz factors of GRB 201015A and GRB 201216C to Γ0 = 204 and
Γ0 = 310, respectively. The present early optical observations are the earliest known observations constraining
outflow parameters and our analysis indicate that VHE detected bursts could have a diverse range of observed
luminosity within the detectable redshift range of present VHE facilities.
