A Confront between <i>Amati</i> and <i>Combo</i> Correlations at Intermediate and Early Redshifts
I consider two gamma-ray burst (GRB) correlations: <i>Amati</i> and <i>Combo</i>. After calibrating them in a cosmology-independent way by employing Beziér polynomials to approximate the Observational Hubble Dataset (OHD), I perform Markov Chain Monte Carlo (MCMC) simulations...
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Format: | Article |
Language: | English |
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MDPI AG
2020-07-01
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Series: | Symmetry |
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Online Access: | https://www.mdpi.com/2073-8994/12/7/1118 |