Showing 1–20 of 22 results
/ Date/ Name
Nov 4, 2025The SPHEREx Satellite MissionSep 30, 2024A physically-motivated template set for high-z galaxy SED fittingSep 19, 2024The relative constraining power of the high-$z$ 21-cm dipole and monopole signalsAug 18, 2023Machine-learning recovery of foreground wedge-removed 21-cm light cones for high-$z$ galaxy mappingOct 10, 2022Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I ObservationsSep 9, 2022Structure Formation and the Global 21-cm Signal in the Presence of Coulomb-like Dark Matter-Baryon InteractionsAug 29, 2022Seeking dark matter with $γ$-ray attenuationAug 26, 2022Balancing the efficiency and stochasticity of star formation with dust extinction in z > 10 galaxies observed by JWSTJan 18, 2022A galaxy-free phenomenological model for the 21-cm power spectrum during reionizationJan 7, 2022Constraining Warm Dark Matter and Pop III stars with the Global 21-cm SignalAug 16, 2021HERA Phase I Limits on the Cosmic 21-cm Signal: Constraints on Astrophysics and Cosmology During the Epoch of ReionizationAug 10, 2020Prospects for distinguishing galaxy evolution models with surveys at redshifts $z \gtrsim 4$May 14, 2020Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation modelsDec 4, 2019Global 21-cm Signal Extraction from Foreground and Instrumental Effects II: Efficient and Self-Consistent Technique for Constraining Nonlinear Signal ModelsOct 22, 2019The Effects of Population III X-ray and Radio Backgrounds on the Cosmological 21-cm SignalSep 27, 2019Astrophysics from the 21-cm backgroundJul 15, 2019A Roadmap for Astrophysics and Cosmology with High-Redshift 21 cm Intensity MappingMar 14, 2019Astro2020 Science White Paper: First Stars and Black Holes at Cosmic Dawn with Redshifted 21-cm ObservationsMar 8, 2018What does the first highly-redshifted 21-cm detection tell us about early galaxies?Oct 6, 2017The Persistence of Population III Star Formation