Mapmaking for precision 21 cm cosmology

Mapmaking for precision 21 cm cosmology

In order to study the “Cosmic Dawn” and the Epoch of Reionization with 21 cm tomography, we need to statistically separate the cosmological signal from foregrounds known to be orders of magnitude brighter. Over the last few years, we have learned much about the role our telescopes play in creating a...

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Bibliographic Details
Main Authors: Liu, Adrian Chi-Yan, Ewall-Wice, Aaron Michael, Hewitt, Jacqueline N., Morales, Miguel F., Parsons, Aaron R., Dillon, Joshua Shane, Tegmark, Max Erik, Neben, Abraham Richard, Zheng, Haoxuan, Ph. D. Massachusetts Institute of Technology
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: American Physical Society 2015
Online Access:http://hdl.handle.net/1721.1/92835
https://orcid.org/0000-0002-4117-570X
https://orcid.org/0000-0001-7776-7240
https://orcid.org/0000-0002-0086-7363
https://orcid.org/0000-0003-3336-9958
https://orcid.org/0000-0001-7670-7190
https://orcid.org/0000-0001-8267-3425

Internet

http://hdl.handle.net/1721.1/92835
https://orcid.org/0000-0002-4117-570X
https://orcid.org/0000-0001-7776-7240
https://orcid.org/0000-0002-0086-7363
https://orcid.org/0000-0003-3336-9958
https://orcid.org/0000-0001-7670-7190
https://orcid.org/0000-0001-8267-3425

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