First limits on the 21 cm power spectrum during the Epoch of X-ray heating
We present first results from radio observations with the Murchison Widefield Array seeking to constrain the power spectrum of 21 cm brightness temperature fluctuations between the redshifts of 11.6 and 17.9 (113 and 75 MHz). 3 h of observations were conducted over two nights with significantly diff...
| Main Authors: | , , , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
2017
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| Online Access: | http://hdl.handle.net/1721.1/108231 https://orcid.org/0000-0002-0086-7363 https://orcid.org/0000-0003-3336-9958 https://orcid.org/0000-0002-4117-570X https://orcid.org/0000-0001-7776-7240 https://orcid.org/0000-0001-7670-7190 https://orcid.org/0000-0003-0422-2324 |