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Autor:
Ould-Boukattine, O. S., Chawla, P., Hessels, J. W. T., Cooper, A. J., Gawroński, M. P., Herrmann, W., Kirsten, F., Hewitt, D. M., Konijn, D. C., Nimmo, K., Pleunis, Z., Puchalska, W., Snelders, M. P.
Fast radio bursts (FRBs) are sufficiently energetic to be detectable from luminosity distances up to at least seven billion parsecs (redshift $z > 1$). Probing the maximum energies and luminosities of FRBs constrains their emission mechanism and cosm
Externí odkaz:
http://arxiv.org/abs/2410.17024
