Investigating temporal features in Swift GRB afterglows: a comparative study of UVOT and XRT data
This study presents a statistical analysis of optical light curves (LCs) of 200 Ultraviolet/Optical Telescope (UVOT)-detected gamma-ray bursts (GRBs) from 2005 to 2018. We have categorized these LCs based on their distinct morphological features, including early flares, bumps, breaks, plateaus, etc....
| Autores: | , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/406272 |
| Acceso en línea: | http://hdl.handle.net/10261/406272 |
| Access Level: | acceso abierto |
| Palabra clave: | Radiation mechanisms: non-thermal Stars: black holes Gamma-ray burst: general Stars: magnetars |
| Sumario: | This study presents a statistical analysis of optical light curves (LCs) of 200 Ultraviolet/Optical Telescope (UVOT)-detected gamma-ray bursts (GRBs) from 2005 to 2018. We have categorized these LCs based on their distinct morphological features, including early flares, bumps, breaks, plateaus, etc. Additionally, to compare features across different wavelengths, we have also included XRT LCs in our sample. The early observation capability of UVOT has allowed us to identify very early flares in 21 GRBs preceding the normal decay or bump, consistent with predictions of external reverse or internal shock. The decay indices of optical LCs following a simple power law (PL) are shallower than corresponding X-ray LCs, indicative of a spectral break between two wavelengths. Not all LCs with PL decay align with the forward shock model and require additional components such as energy injection or a structured jet. Further, plateaus in the optical LCs are primarily consistent with energy injection from the central engine to the external medium. However, in four cases, plateaus followed by steep decay may have an internal origin. The optical luminosity observed during the plateau is tightly correlated with the break time, indicative of a magnetar as their possible central engine. For LCs with early bumps, the peak position, correlations between the parameters, and observed achromaticity allowed us to constrain their origin as the onset of afterglow, off-axis jet, late re-brightening, etc. In conclusion, the ensemble of observed features is explained through diverse physical mechanisms or emissions observed from different outflow locations and, in turn, diversity among possible progenitors. © The Author(s) 2025. Published by Oxford University Press on behalf of Royal Astronomical Society. |
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