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High redshift Gamma-Ray Bursts

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arxiv 1503.03072 v1 pith:EEKH36ZY submitted 2015-03-10 astro-ph.CO astro-ph.HE

R. Salvaterra This is my paper
classification astro-ph.COastro-ph.HE
keywords burstsgamma-raygrbsredshiftallowcollectcomplementarydiscuss
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Ten years of operations of the Swift satellite have allow us to collect a small sample of long Gamma-Ray Bursts (GRBs) at redshift larger than six. I will review here the present status of this research field and discuss the possible use of GRBs as a fundamental new tool to explore the early Universe, complementary to quasar and galaxy surveys.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Tightening Bounds on Warm Dark Matter with High-Redshift Gamma-Ray Bursts

    astro-ph.HE 2026-07 conditional novelty 4.0 of 10

    Using the redshift distribution of 118 luminous Swift GRBs, warm dark matter particles are bounded to mx ≥ 1.3 keV at 95% CL (≥3.4 keV if GRBs exactly trace the SFR).

  2. Gamma-ray bursts reveal the history and faint contributors of cosmic reionization

    astro-ph.CO 2026-07 conditional novelty 4.0 of 10

    Long gamma-ray bursts imply a higher cosmic star formation rate density at z>6 than galaxy surveys detect, sufficient to drive reionization with moderate ionizing efficiency and escape fraction, implying a large popul...

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