Using 21 cm absorption surveys to measure the average H i spin temperature in distant galaxies
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/462/2/1341/8009171/stw1722.pdf
Reference102 articles.
1. Discovery of H i gas in a young radio galaxy at z = 0.44 using the Australian Square Kilometre Array Pathfinder
2. Astropy: A community Python package for astronomy
3. On the Possibility of Detecting Redshifted 21-CM Absorption Lines in the Spectra of Quasi-Stellar Sources
4. On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties
5. The cosmic evolution of radio-AGN feedback to z = 1
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1. Detections of 21 cm absorption with a blind FAST survey at z ≤ 0.09;Astronomy & Astrophysics;2023-06-29
2. H i absorption associated with Norma’s brightest cluster galaxy;Monthly Notices of the Royal Astronomical Society;2022-12-19
3. Deep ASKAP EMU Survey of the GAMA23 field: properties of radio sources;Monthly Notices of the Royal Astronomical Society;2022-04-11
4. The First Large Absorption Survey in H i (FLASH): I. Science goals and survey design;Publications of the Astronomical Society of Australia;2022
5. Extragalactic H i 21-cm absorption line observations with the Five-hundred-meter Aperture Spherical radio Telescope;Monthly Notices of the Royal Astronomical Society;2021-03-19
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