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Spatial distribution of the gamma-ray bursts at very high redshift

Published online by Cambridge University Press:  08 May 2018

Attila Mészáros Open the ORCID record for Attila Mészáros [Opens in a new window]
Attila Mészáros*
Affiliation:
Charles University, Faculty of Mathematics and Physics, Astronomical Institute, V Holešovičkách 2, Prague 8, Czech Republic, email:[email protected]
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Abstract

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The author - with his collaborators - already in years 1995-96 have shown - purely from the analyses of the observations - that the gamma-ray bursts (GRBs) can be till redshift 20. Since that time several other statistical studies of the spatial distribution of GRBs were provided. Remarkable conclusions concerning the star-formation rate and the validity of the cosmological principle were obtained about the regions of the cosmic dawn. In this contribution these efforts are surveyed.

Keywords

Cosmology: large-scale structure of the UniverseobservationsmiscellaneousStars: gamma-ray bursts
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S333: Peering towards Cosmic Dawn , October 2017 , pp. 203 - 206
Copyright
Copyright © International Astronomical Union 2018 

References

Abbott, B. P. et al. 2017 ApJL, 848, L13Google Scholar
Bagoly, Z., et al. 2003, A&A, 398, 919Google Scholar
Bagoly, Z. et al. 2016a, Galaxies at High Redshift and Their Evolution Over Cosmic Time, IAU Symp., 319, 2Google Scholar
Bagoly, Z. et al. 2016b, Galaxies at High Redshift and Their Evolution Over Cosmic Time, IAU Symp., 319, 3Google Scholar
Balázs, L. G., Mészáros, A., & Horváth, I., 1998, A&A, 339, 1Google Scholar
Balázs, L. G., et al. 1999, A&AS, 138, 417Google Scholar
Balázs, L. G., et al. 2015, MNRAS, 452, 2236Google Scholar
Birch, P., 1982, Nature, 298, 451CrossRefGoogle Scholar
Carroll, S. M., Press, W. H., & Turner, E. L., 1992, ARAA, 30, 499Google Scholar
Clowes, R. G., et al. 2013, MNRAS, 429, 2910CrossRefGoogle Scholar
Collins, C. B. & Hawking, S. W., 1973, MNRAS, 162, 307Google Scholar
Costa, E., et al. 1997, Nature, 387, 783Google Scholar
Goldstein, A., et al. 2013, ApJS, 208, 21Google Scholar
Horváth, I., Mészáros, P., & Mészáros, A., 1996, ApJ, 470, 56CrossRefGoogle Scholar
Horváth, I., Hakkila, J., & Bagoly, Z., 2014, A&A, 561, L12Google Scholar
Horváth, I., et al. 2015, A&A, 584, A48Google Scholar
Klebesadel, R. W., Strong, I. B., & Olson, R. A., 1973, ApJ, 182, L85Google Scholar
Levan, A. J., et al. 2014, ApJ, 781, 13CrossRefGoogle Scholar
Mazets, E. P., et al. 1981, Ap&SS, 80, 3Google Scholar
Meegan, C. A., et al. 1992, Nature, 355, 143Google Scholar
Mészáros, A. & Mészáros, P., 1996, ApJ, 466, 29Google Scholar
Mészáros, A., Bagoly, Z, & Vavrek, R., 2000a, A&A, 354, 1Google Scholar
Mészáros, A., et al. 2000b, ApJ, 539, 98Google Scholar
Mészáros, A. & Štoček, J., 2003, A&A, 403, 443Google Scholar
Mészáros, A. et al. 2006 A&A, 455, 785Google Scholar
Mészáros, A. et al., 2009a, Baltic Astronomy, 18, 293Google Scholar
Mészáros, A., et al. 2009b, Sixth Huntsville GRB Symposium, AIP Conf. Proc., 1133, 483Google Scholar
Mészáros, A., et al. 2011, A&A, 529, A55Google Scholar
Mészáros, P. & Mészáros, A., 1995, ApJ, 49, 9Google Scholar
Paczyński, B., 1986, ApJL, 308, L43CrossRefGoogle Scholar
Perley, D. 2017, http://www.astro.caltech.edu/grbox/grbox.phpGoogle Scholar
Peebles, P. J. E. 1993, Principles of Physical Cosmology (Princeton University Press)Google Scholar
Reichart, D. E. & Mészáros, P., 1997, ApJ, 483, 597Google Scholar
Řípa, J. & Mészáros, A., 2016, Ap&SS, 361, 370Google Scholar
Řípa, J. & Shafieloo, A., 2017, ApJ, 851, 15Google Scholar
Rudnick, L., Brown, S. & Williams, L. R. 2007, ApJ, 671, 40; Errata: ApJ, 678, 1531 (2008)Google Scholar
Sokolov, I. V. et al. 2015, Quark Phase Transition in Compact Objects, SAO, Russia, 111Google Scholar
Tanvir, N. R., et al. 2013, Nature, 500, 537Google Scholar
Tarnopolski, M., 2017, MNRAS, 472, 4819Google Scholar
Tegmark, M., et al. 1996, ApJ, 468, 214Google Scholar
Usov, N. V. & Chibisov, G. V., 1975, Soviet Astronomy, 19, 115Google Scholar
Vavrek, R., et al. 2008, MNRAS, 391, 1741Google Scholar
Verkhodanov, O. V. et al. 2015, Quark Phase Transition in Compact Objects, SAO, Russia, 142Google Scholar
Weinberg, S. 1972, Gravitation and Cosmology (J.Wiley, New York - London - Sydney - Toronto)Google Scholar
Woosley, S. E. & Bloom, J. S., 2006, ARAA, 44, 507Google Scholar
Yadav, J. K., Bagla, J. S., & Khandai, N., 2010, MNRAS, 405, 2009Google Scholar