CONFIRMATION OF WIDE-FIELD SIGNATURES IN REDSHIFTED 21 cm POWER SPECTRA
We confirm our recent prediction of the "pitchfork" foreground signature in power spectra of high-redshift 21 cm measurements where the interferometer is sensitive to large-scale structure on all baselines. This is due to the inherent response of a wide-field instrument and is characterize...
Auteurs principaux: | , , , , , , , , , , , |
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Autres auteurs: | |
Format: | Article |
Langue: | en_US |
Publié: |
IOP Publishing
2015
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Accès en ligne: | http://hdl.handle.net/1721.1/98375 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/0000-0003-3336-9958 https://orcid.org/0000-0001-7670-7190 https://orcid.org/0000-0003-0422-2324 |
Internet
http://hdl.handle.net/1721.1/98375https://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/0000-0003-3336-9958
https://orcid.org/0000-0001-7670-7190
https://orcid.org/0000-0003-0422-2324