Deep Neural Networks for Estimation of Gamma-Ray Burst Redshifts
arXiv:2401.11005 · doi:10.1093/mnras/stae535
Abstract
While the available set of Gamma-ray Burst (GRB) data with known redshift is currently limited, a much larger set of GRB data without redshift is available from different instruments. This data includes well-measured prompt gamma-ray flux and spectral information. We estimate the redshift of a selection of these GRBs detected by Fermi-GBM and Konus-Wind using Machine Learning techniques that are based on spectral parameters. We find that Deep Neural Networks with Random Forest models employing non-linear relations among input parameters can reasonably reproduce the pseudo-redshift distribution of GRBs, mimicking the distribution of GRBs with spectroscopic redshift. Furthermore, we find that the pseudo-redshift samples of GRBs satisfy (i) Amati relation between the peak photon energy of the time-averaged energy spectrum in the cosmological rest frame of the GRB and the isotropic-equivalent radiated energy during the prompt phase; and (ii) Yonetoku relation between and isotropic-equivalent luminosity , both measured during the peak flux interval.
10 pages, 7 figures, accepted in MNRAS
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Cited by in corpus (6)
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- Gamma-ray Bursts as Distance Indicators by a Statistical Learning Approach
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