… reverse shock emission dominates in the radio/millimeter and at ≲ 0.1 days in the UV/optical/NIR,
while the forward shock … Using the combined forward and reverse shock emission, we …

… , which we attribute to emission from a reverse shock. The VLA observations above 24 GHz
and … component, which we associate with underlying forward shock emission (Section 3.1). …

… and characterization of an RS in GRB 130427A, and highlights the importance of rapid-response
radio observations in the study of the properties and dynamics of GRB ejecta. …

… The optical light curve of GRB 180418A can be modeled by forward shock (FS) plus
reverse shock (RS). We fit the light curves with standard external shock models and derive the …

… give a brief description of GRB 130427A observations; in Section 3 … shocks (forward and
reverse) that evolve adiabatically in a stellar wind with the quantities observed in GRB 130427A; …

… The complex multiwavelength emission of gamma-ray burst (GRB) afterglow 130427A (…
for by a hybrid reverse–forward shock synchrotron model, with inverse-Compton emerging only …

… The reverse shock emission during the third injection episode is not shown and would be
dimmer than that of the forward shock, if the reverse shock has the same microphysical …

… , 081007, 090102, 090424, and 130427A. By modeling their optical afterglows with …
forward-shock emission at late times (>10 ks). We find that GRBs with an identifiable reverse-shock …

… GRBs similar in nature to GRB 130427A, inhabiting low-density media and exhibiting strong
reverse shocks, are probably not uncommon but may have been difficult to recognize in the …

… results indicate that GRB 180720B is the very first GRB event … the reverse shock in the early
phase and the forward shock … of the reverse shock compared with the forward shock due to …