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- W2030759009 abstract "Early observations of 15 GRB afterglows taken (2008–09) by ROTSE‐III along with the published data of 26 others have been used to study the rising temporal nature seen at optical frequencies. A good fraction of early time temporal rising indices found to be flatter than the model predicted values. Under the assumptions of “onset of the afterglow”, the peak times of the rising optical light curves have been used to estimate the initial Lorentz factor Γ0 of the fireball, ranging from ∼100 to ∼1000. The estimated values of Γ0 seems correlated with the isotropic equivalent gamma‐ray energies of GRBs i.e. highly energetic GRBs have higher values of Γ0. The analysis also indicates that for a larger sample of GRBs, the peak times of the rising afterglow light curves and the derived values of the initial Lorentz factors along with the respective prompt emission properties like Epeak can be used to better constrain possible scenarios like off‐axis emission and structured outflow." @default.
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- W2030759009 date "2011-01-01" @default.
- W2030759009 modified "2023-10-16" @default.
- W2030759009 title "Early ROTSE-III observations of GRB afterglows" @default.
- W2030759009 doi "https://doi.org/10.1063/1.3621761" @default.
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