FOREGROUNDS IN WIDE-FIELD REDSHIFTED 21 cm POWER SPECTRA
Detection of 21 cm emission of H i from the epoch of reionization, at redshifts z > 6, is limited primarily by foreground emission. We investigate the signatures of wide-field measurements and an all-sky foreground model using the delay spectrum technique that maps the measurements to foreground...
Main Authors: | , , , , , , , , , , , , , , , , |
---|---|
Other Authors: | |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2015
|
Online Access: | http://hdl.handle.net/1721.1/97096 https://orcid.org/0000-0002-4117-570X https://orcid.org/0000-0001-7776-7240 https://orcid.org/0000-0001-7130-208X https://orcid.org/0000-0002-0086-7363 https://orcid.org/0000-0003-1941-7458 https://orcid.org/0000-0003-3336-9958 https://orcid.org/0000-0001-7670-7190 https://orcid.org/0000-0003-0422-2324 |
Internet
http://hdl.handle.net/1721.1/97096https://orcid.org/0000-0002-4117-570X
https://orcid.org/0000-0001-7776-7240
https://orcid.org/0000-0001-7130-208X
https://orcid.org/0000-0002-0086-7363
https://orcid.org/0000-0003-1941-7458
https://orcid.org/0000-0003-3336-9958
https://orcid.org/0000-0001-7670-7190
https://orcid.org/0000-0003-0422-2324