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Paper: The Early X-ray Afterglows of Optical Transient and Dark GRBs
Volume: 373, The Central Engine of Active Galactic Nuclei
Page: 749
Authors: Lin, Y.-Q.
Abstract: We show that the distribution of the X-ray, the γ-ray and the fox of the dark GRBs and OT GRBs are similar; any observed differences should simply be due to statistical fluctuation. These results indicate that the suppression of optical emission in the dark GRBs should result from circumburst environment, not from their central engine.
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