The 21-cm bispectrum as a probe of non-Gaussianities due to X-ray heating

Author:

Watkinson Catherine A1ORCID,Giri Sambit K2ORCID,Ross Hannah E23ORCID,Dixon Keri L34ORCID,Iliev Ilian T3ORCID,Mellema Garrelt2ORCID,Pritchard Jonathan R1

Affiliation:

1. Department of Physics, Blackett Laboratory, Imperial College, London, SW7 2AZ, UK

2. Department of Astronomy and Oskar Klein Centre, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden

3. Astronomy Centre, Department of Physics & Astronomy, Pevensey III Building, University of Sussex, Falmer, Brighton, BN1 9QH, UK

4. New York University Abu Dhabi, PO Box 129188, Saadiyat Island, Abu Dhabi, UAE

Funder

European Research Council

Science and Technology Facilities Council

Swedish Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. Inferring astrophysical parameters using the 2D cylindrical power spectrum from reionization;Monthly Notices of the Royal Astronomical Society;2024-08-17

2. How informative are summaries of the cosmic 21 cm signal?;Astronomy & Astrophysics;2024-08

3. Inverse Gertsenshtein effect as a probe of high-frequency gravitational waves;Journal of Cosmology and Astroparticle Physics;2024-05-01

4. A covariant formulation for cosmological radiative transfer of the 21-cm line;Monthly Notices of the Royal Astronomical Society;2024-04-23

5. The long-lasting effect of X-ray pre-heating in the post-reionization intergalactic medium;Monthly Notices of the Royal Astronomical Society;2024-03-15

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