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 …
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 …
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 …
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 …
The patchiness in the reionization process alters the statistics of cosmic microwave background (CMB), with the kinematic Sunyaev–Zeldovich (kSZ) effect in the CMB …
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 …
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 …
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) …
In this thesis, I describe several advances in modelling sources of systematic error associated with microwave telescope optics. Microwave telescopes observing the Cosmic …