Inferring reionization and galaxy properties from the patchy kinetic Sunyaev–Zel'dovich signal

I Nikolić, A Mesinger, Y Qin… - Monthly Notices of the …, 2023 - academic.oup.com
ABSTRACT The patchy kinetic Sunyaev–Zel'dovich (kSZ) signal is an integral probe of the
timing and morphology of the epoch of reionization (EoR). Recent observations have …

Constraining cosmic reionization by combining the kinetic Sunyaev–Zel'dovich and the 21 cm power spectra

I Georgiev, A Gorce, G Mellema - Monthly Notices of the Royal …, 2024 - academic.oup.com
ABSTRACT During the Epoch of Reionization (EoR), the ultraviolet radiation from the first
stars and galaxies ionized the neutral hydrogen of the intergalactic medium, which can emit …

Snowmass2021 Cosmic Frontier White Paper: 21cm Radiation as a Probe of Physics Across Cosmic Ages

A Liu, L Newburgh, B Saliwanchik, A Slosar - arXiv preprint arXiv …, 2022 - arxiv.org
The 21cm line refers to a forbidden transition in neutral hydrogen associated with alignment
of spins of the proton and electron. It is a very low energy transition that is emitted whenever …

Correlation-based Beam Calibration of 21 cm Intensity Mapping

J Ding, X Wang, UL Pen, XD Li - The Astrophysical Journal …, 2024 - iopscience.iop.org
Foreground removal presents a significant obstacle in both current and forthcoming intensity-
mapping surveys. While numerous techniques have been developed that show promise in …

A general Bayesian framework to account for foreground map errors in global 21-cm experiments

M Pagano, P Sims, A Liu, D Anstey… - Monthly Notices of …, 2024 - academic.oup.com
Measurement of the global 21-cm signal during Cosmic Dawn and the Epoch of
Reionization is made difficult by bright foreground emission which is 2–5 orders of …

Probing the physics of reionization using kinematic Sunyaev–Zeldovich power spectrum from current and upcoming cosmic microwave background surveys

D Jain, TR Choudhury, S Raghunathan… - Monthly Notices of the …, 2024 - academic.oup.com
The patchiness in the reionization process alters the statistics of cosmic microwave
background (CMB), with the kinematic Sunyaev–Zeldovich (kSZ) effect in the CMB …

Forecasts and Statistical Insights for Line Intensity Mapping Cross-correlations: A Case Study with 21 cm×[C ii]

H Fronenberg, A Liu - The Astrophysical Journal, 2024 - iopscience.iop.org
Intensity mapping—the large-scale mapping of selected spectral lines without resolving
individual sources—is quickly emerging as an efficient way to conduct large cosmological …

Tackling the Challenges in the 21 cm Global Spectrum Experiment: The Impact of Ionosphere and Beam Distortion

Y Wang, X Wang, S Sun, F Wu, S Luo… - The Astrophysical …, 2024 - iopscience.iop.org
The H i 21 cm global signal from the Cosmic Dawn and the Epoch of Reionization (EoR)
offers critical insights into the evolution of our Universe. Yet, its detection presents significant …

Retrieving cosmological information from small-scale CMB foregrounds-II. The kinetic Sunyaev Zel'dovich effect

A Gorce, M Douspis, L Salvati - Astronomy & Astrophysics, 2022 - aanda.org
Recent results of ground-based telescopes, giving high-quality measurements of the cosmic
microwave background (CMB) temperature power spectrum on small scales (below 1 deg) …

Polarized beams and the things they've seen: Modelling optical systematics for CMB polarisation experiments

AE Adler - 2024 - diva-portal.org
In this thesis, I describe several advances in modelling sources of systematic error
associated with microwave telescope optics. Microwave telescopes observing the Cosmic …