The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Gamma‐Ray Burst Formation Rate Inferred from the Spectral Peak Energy–Peak Luminosity Relation
Open accessAbstract
We estimate a gamma-ray burst (GRB) formation rate based on the new relation between the spectral peak energy ( E p ) and the peak luminosity. The new relation is derived by combining the data of E p and the peak luminosities by BeppoSAX and BATSE, and it looks considerably tighter and more reliable than the relations suggested by the previous works. Using the new E p -luminosity relation, we estimate redshifts of the 689 GRBs without known distances in the BATSE catalog and derive a GRB formation rate as a function of the redshift. For the redshift range of 0 ≤ z ≤ 2, the GRB formation rate increases and is well correlated with the star formation rate, while it keeps constant toward z ~ 12. We also discuss the luminosity function and the redshift dependence of the intrinsic luminosity (luminosity evolution).
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Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., Limon, M., Meyer, S. S., Page, L., Spergel, D. N., Tucker, G. S., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377253 · Cited by 4,860
Cited by
The physics of gamma-ray bursts & relativistic jets
Kumar, P., & Zhang, B. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.09.008 · Cited by 952
Di Valentino, E., Said, J. L., Riess, A., Pollo, A., Poulin, V., Gómez-Valent, A., Weltman, A., Palmese, A., Huang, C. D., Bruck, C. V. D., et al. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.101965 · Cited by 319
Butler, N. R., Kocevski, D., Bloom, J. S., & Curtis, J. L. (2007) · The Astrophysical Journal · doi:10.1086/522492 · Cited by 278
THE AFTERGLOWS OF SWIFT-ERA GAMMA-RAY BURSTS. II. TYPE I GRB VERSUS TYPE II GRB OPTICAL AFTERGLOWS
Kann, D. A., Klose, S., Zhang, B., Covino, S., Butler, N. R., Malesani, D., Nakar, E., Wilson, A. C., Antonelli, L. A., Chincarini, G., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/734/2/96 · Cited by 276
Zhang, B.-B., Zhang, B., Liang, E.-W., Fan, Y.-Z., Wu, X.-F., Pe'er, A., Maxham, A., Gao, H., & Dong, Y.-M. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/730/2/141 · Cited by 259
Metadata
- Authors
- Yonetoku, D., Murakami, T., Nakamura, T., Yamazaki, R., Inoue, A. K., & Ioka, K.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2004-07-10
- Volume
- 609
- Issue
- 2
- Pages
- 935-951
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2086775208
- Cited by
- 712
- References
- 2
- FWCI
- 14.97
- Type
- journal article
- Language
- en
- Open access
- bronze
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