Simulating the 21 cm forest detectable with LOFAR and SKA in the spectra of high-z GRBs

Simulating the 21 cm forest detectable with LOFAR and SKA in the spectra of high-z GRBs

We investigate the feasibility of detecting 21 cm absorption features in the afterglow spectra of high redshift long Gamma Ray Bursts (GRBs). This is done employing simulations of cosmic reionization, together with estimates of the GRB radio afterglow flux and the instrumental characteristics of the...

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Bibliographic Details
Main Authors: Ciardi, B., Inoue, S., Abdalla, F.B., Asad, K., Bernardi, G., Bolton, James S., Brentjens, M., de Bruyn, A.G., Chapman, E., Daiboo, S., Fernandez, E.R., Ghosh, A., Graziani, L., Harker, G.J.A., Iliev, I.T., Jelic, V., Jensen, H., Kazemi, S., Koopmans, L.V.E., Martinez, O., Maselli, A., Mellema, G., Offringa, A.R., Pandey, V.N., Schaye, Joop, Thomas, R., Vedantham, H., Yatawatta, S., Zaroubi, S.
Format: Article
Published: Oxford University Press 2015
Subjects:
gamma-ray burst: general
dark ages
reionization
first stars
radio lines: general
Online Access:https://eprints.nottingham.ac.uk/42512/

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