Using 21 cm absorption surveys to measure the average H I spin temperature in distant galaxies

We present a statistical method for measuring the average H I spin temperature in distant galaxies using the expected detection yields from future wide-field 21 cm absorption surveys. As a demonstrative case study, we consider an all-southern-sky simulated survey of 2-h per pointing with the Austral...

詳細記述

書誌詳細
主要な著者: Allison, J, Zwaan, M, Duchesne, S, Curran, S
フォーマット: Journal article
言語:English
出版事項: Oxford University Press 2016