The Optical Light Curve of GRB 221009A: The Afterglow and the Emerging Supernova Article Swipe
YOU?
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· 2023
· Open Access
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· DOI: https://doi.org/10.3847/2041-8213/acc101
We present extensive optical photometry of the afterglow of GRB 221009A. Our data cover 0.9–59.9 days from the time of Swift and Fermi gamma-ray burst (GRB) detections. Photometry in rizy -band filters was collected primarily with Pan-STARRS and supplemented by multiple 1–4 m imaging facilities. We analyzed the Swift X-ray data of the afterglow and found a single decline rate power law f ( t ) ∝ t −1.556±0.002 best describes the light curve. In addition to the high foreground Milky Way dust extinction along this line of sight, the data favor additional extinction to consistently model the optical to X-ray flux with optically thin synchrotron emission. We fit the X-ray-derived power law to the optical light curve and find good agreement with the measured data up to 5−6 days. Thereafter we find a flux excess in the riy bands that peaks in the observer frame at ∼20 days. This excess shares similar light-curve profiles to the Type Ic broad-lined supernovae SN 2016jca and SN 2017iuk once corrected for the GRB redshift of z = 0.151 and arbitrarily scaled. This may be representative of an SN emerging from the declining afterglow. We measure rest-frame absolute peak AB magnitudes of M g = −19.8 ± 0.6 and M r = − 19.4 ± 0.3 and M z = −20.1 ± 0.3. If this is an SN component, then Bayesian modeling of the excess flux would imply explosion parameters of M ⊙ , M ⊙ , and km s −1 , for the ejecta mass, nickel mass, and ejecta velocity respectively, inferring an explosion energy of E kin ≃ 2.6–9.0 × 10 52 erg.
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- en
- Landing Page
- https://doi.org/10.3847/2041-8213/acc101
- https://iopscience.iop.org/article/10.3847/2041-8213/acc101/pdf
- OA Status
- gold
- Cited By
- 38
- References
- 60
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4361216445
Raw OpenAlex JSON
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https://openalex.org/W4361216445Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/2041-8213/acc101Digital Object Identifier
- Title
-
The Optical Light Curve of GRB 221009A: The Afterglow and the Emerging SupernovaWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
-
2023Year of publication
- Publication date
-
2023-03-01Full publication date if available
- Authors
-
M. Fulton, S. J. Smartt, Lauren Rhodes, M. E. Huber, V. Ashley Villar, T. Moore, Shubham Srivastav, A. S. B. Schultz, K. C. Chambers, L. Izzo, J. Hjorth, T. W. Chen, M. Nicholl, R. J. Foley, A. Rest, K. Smith, D. R. Young, Stuart Sim, Joe Bright, Yossef Zenati, Thomas de Boer, J. Bulger, J. Fairlamb, Hua Gao, Chien-Cheng Lin, T. Lowe, E. A. Magnier, I. A. Smith, R. J. Wainscoat, D. A. Coulter, D. O. Jones, C. D. Kilpatrick, Peter McGill, E. Ramirez‐Ruiz, Kyoung-Soo Lee, Gautham Narayan, Vandana Ramakrishnan, Ryan Ridden-Harper, Akriti Singh, Qinan Wang, A. K. H. Kong, Chow‐Choong Ngeow, Y. C. Pan, S. Yang, Kyle W. Davis, Anthony L. Piro, C. Rojas-Bravo, Julian S. Sommer, S. K. YadavalliList of authors in order
- Landing page
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https://doi.org/10.3847/2041-8213/acc101Publisher landing page
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https://iopscience.iop.org/article/10.3847/2041-8213/acc101/pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://iopscience.iop.org/article/10.3847/2041-8213/acc101/pdfDirect OA link when available
- Concepts
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Physics, Afterglow, Light curve, Astrophysics, Gamma-ray burst, Supernova, Photometry (optics), Redshift, Galaxy, Power law, Milky Way, Flux (metallurgy), Stars, Extinction (optical mineralogy), Astronomy, Optics, Materials science, Metallurgy, Mathematics, StatisticsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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38Total citation count in OpenAlex
- Citations by year (recent)
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2025: 13, 2024: 17, 2023: 8Per-year citation counts (last 5 years)
- References (count)
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60Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.modeling | 229 |
| abstract_inverted_index.multiple | 41 |
| abstract_inverted_index.observer | 145 |
| abstract_inverted_index.profiles | 155 |
| abstract_inverted_index.redshift | 172 |
| abstract_inverted_index.velocity | 337 |
| abstract_inverted_index.2.6–9.0 | 347 |
| abstract_inverted_index.<mml:math | 239, 268, 298 |
| abstract_inverted_index.afterglow | 8, 54 |
| abstract_inverted_index.agreement | 122 |
| abstract_inverted_index.collected | 34 |
| abstract_inverted_index.corrected | 168 |
| abstract_inverted_index.declining | 190 |
| abstract_inverted_index.describes | 71 |
| abstract_inverted_index.emission. | 107 |
| abstract_inverted_index.explosion | 236, 341 |
| abstract_inverted_index.extensive | 3 |
| abstract_inverted_index.gamma-ray | 24 |
| abstract_inverted_index.inferring | 339 |
| abstract_inverted_index.optically | 104 |
| abstract_inverted_index.primarily | 35 |
| abstract_inverted_index.0.9–59.9 | 15 |
| abstract_inverted_index.<mml:mrow> | 243, 246, 252, 255, 259, 272, 275, 281, 284, 288, 302, 305, 311, 315, 319 |
| abstract_inverted_index.<mml:msub> | 242, 271, 301 |
| abstract_inverted_index.Pan-STARRS | 37 |
| abstract_inverted_index.Photometry | 28 |
| abstract_inverted_index.Thereafter | 131 |
| abstract_inverted_index.additional | 93 |
| abstract_inverted_index.afterglow. | 191 |
| abstract_inverted_index.component, | 226 |
| abstract_inverted_index.extinction | 84, 94 |
| abstract_inverted_index.foreground | 80 |
| abstract_inverted_index.magnitudes | 198 |
| abstract_inverted_index.parameters | 237 |
| abstract_inverted_index.photometry | 5 |
| abstract_inverted_index.rest-frame | 194 |
| abstract_inverted_index.supernovae | 161 |
| abstract_inverted_index.</mml:math> | 264, 293, 324 |
| abstract_inverted_index.</mml:mrow> | 245, 248, 254, 258, 262, 274, 277, 283, 287, 291, 304, 307, 314, 318, 322 |
| abstract_inverted_index.</mml:msub> | 249, 278, 308 |
| abstract_inverted_index.arbitrarily | 178 |
| abstract_inverted_index.broad-lined | 160 |
| abstract_inverted_index.detections. | 27 |
| abstract_inverted_index.facilities. | 45 |
| abstract_inverted_index.light-curve | 154 |
| abstract_inverted_index.synchrotron | 106 |
| abstract_inverted_index.consistently | 96 |
| abstract_inverted_index.supplemented | 39 |
| abstract_inverted_index.<mml:msubsup> | 251, 280, 310 |
| abstract_inverted_index.X-ray-derived | 111 |
| abstract_inverted_index.respectively, | 338 |
| abstract_inverted_index.</mml:msubsup> | 263, 292, 323 |
| abstract_inverted_index.representative | 183 |
| abstract_inverted_index.−1.556±0.002 | 69 |
| abstract_inverted_index.<mml:mi>M</mml:mi> | 244, 273 |
| abstract_inverted_index.<mml:mi>v</mml:mi> | 303 |
| abstract_inverted_index.<mml:mo>+</mml:mo> | 260, 289, 320 |
| abstract_inverted_index.<mml:mo>=</mml:mo> | 250, 279, 309 |
| abstract_inverted_index.overflow="scroll"> | 241, 270, 300 |
| abstract_inverted_index.<mml:mi>Ni</mml:mi> | 276 |
| abstract_inverted_index.<mml:mi>ej</mml:mi> | 247, 306 |
| abstract_inverted_index.<mml:mn>0.4</mml:mn> | 286 |
| abstract_inverted_index.<mml:mn>0.6</mml:mn> | 290 |
| abstract_inverted_index.<mml:mn>1.0</mml:mn> | 282 |
| abstract_inverted_index.<mml:mn>1.7</mml:mn> | 257 |
| abstract_inverted_index.<mml:mn>2.4</mml:mn> | 261 |
| abstract_inverted_index.<mml:mn>7.1</mml:mn> | 253 |
| abstract_inverted_index.<mml:mo>−</mml:mo> | 256, 285, 316 |
| abstract_inverted_index.<mml:mn>5700</mml:mn> | 317 |
| abstract_inverted_index.<mml:mn>5900</mml:mn> | 321 |
| abstract_inverted_index.mathvariant="normal">33,900</mml:mi> | 313 |
| abstract_inverted_index.xmlns:mml="http://www.w3.org/1998/Math/MathML" | 240, 269, 299 |
| cited_by_percentile_year.max | 100 |
| cited_by_percentile_year.min | 99 |
| corresponding_author_ids | https://openalex.org/A5019060538 |
| countries_distinct_count | 9 |
| institutions_distinct_count | 49 |
| corresponding_institution_ids | https://openalex.org/I126231945 |
| citation_normalized_percentile.value | 0.98205921 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |