Constraining the Reionization Process via 21-cm Power Spectra
碩士 === 國立臺灣大學 === 天文物理研究所 === 102 === Up to date there has been little observational constraints on the cosmic reionization process, the phase transition of the universe caused by the for- mation of the first luminous objects. Current theoretical modelling of reion- ization is subject to large uncer...
Main Authors: | Fang-Chun Liu, 劉芳君 |
---|---|
Other Authors: | Tzu-Ching Chang |
Format: | Others |
Language: | en_US |
Published: |
2014
|
Online Access: | http://ndltd.ncl.edu.tw/handle/46893488581119280773 |
Similar Items
-
Probing the epoch of reionization with redshifted 21 cm HI emission
by: Bowman, Judd D. (Judd David)
Published: (2009) -
Reionization and beyond: detecting the peaks of the cosmological 21 cm signal
by: Mesinger, Andrei, et al.
Published: (2019) -
PAPER-64 CONSTRAINTS ON REIONIZATION: THE 21 cm POWER SPECTRUM AT z = 8.4
by: Ali, Zaki S., et al.
Published: (2015) -
The Role of the Instrumental Response in 21 cm Epoch of Reionization Power Spectrum Gridding Analyses
by: Barry, N., et al.
Published: (2022) -
Measuring the 21cm Power Spectrum from the Epoch of Reionization with the Giant Metrewave Radio Telescope
by: Paciga, Gregory
Published: (2013)