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First limits on the 21 cm power spectrum during the Epoch of X-ray heating
- Source :
- arXiv, Monthly Notices of the Royal Astronomical Society, 460(4), 4320-4347. Oxford University Press, Monthly Notices of the Royal Astronomical Society
- Publication Year :
- 2017
-
Abstract
- 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 different levels of ionospheric activity. We use these data to assess the impact of systematic errors at low frequency, including the ionosphere and radio-frequency interference, on a power spectrum measurement. We find that after the 1–3 h of integration presented here, our measurements at the Murchison Radio Observatory are not limited by RFI, even within the FM band, and that the ionosphere does not appear to affect the level of power in the modes that we expect to be sensitive to cosmology. Power spectrum detections, inconsistent with noise, due to fine spectral structure imprinted on the foregrounds by reflections in the signal-chain, occupy the spatial Fourier modes where we would otherwise be most sensitive to the cosmological signal. We are able to reduce this contamination using calibration solutions derived from autocorrelations so that we achieve an sensitivity of 104 mK on comoving scales k ≲ 0.5 h Mpc[superscript −1]. This represents the first upper limits on the 21 cm power spectrum fluctuations at redshifts 12 ≲ z ≲ 18 but is still limited by calibration systematics. While calibration improvements may allow us to further remove this contamination, our results emphasize that future experiments should consider carefully the existence of and their ability to calibrate out any spectral structure within the EoR window.<br />National Science Foundation (U.S.) (AST-0457585)<br />National Science Foundation (U.S.) (AST-0821321)<br />National Science Foundation (U.S.) (AST-1105835)<br />National Science Foundation (U.S.) (AST-1410719)<br />National Science Foundation (U.S.) (AST-1410484)<br />National Science Foundation (U.S.) (AST-1411622)<br />National Science Foundation (U.S.) (AST-1440343)<br />National Science Foundation (U.S.) (1122374)<br />National Science Foundation (U.S.) (PHY-0835713)<br />National Science Foundation (U.S.) (CAREER-0847753)<br />National Science Foundation (U.S.) (AST-0908884)<br />United States. Air Force Office of Scientific Research (FA9550-0510247)
- Subjects :
- dark age
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
media_common.quotation_subject
first stars
FOS: Physical sciences
Library science
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
Settore FIS/05 - Astronomia e Astrofisica
Excellence
0103 physical sciences
media_common.cataloged_instance
European union
IBM
dark ages
Instrumentation and Methods for Astrophysics (astro-ph.IM)
010303 astronomy & astrophysics
Investment fund
media_common
Physics
Government
010308 nuclear & particles physics
European research
first star
Astrophysics::Instrumentation and Methods for Astrophysics
Astronomy and Astrophysics
interferometric [techniques]
galaxies [X-rays]
X-rays: galaxies
13. Climate action
Space and Planetary Science
techniques: interferometric
general [radio lines]
Commonwealth
reionization
Christian ministry
Astrophysics - Instrumentation and Methods for Astrophysics
radio lines: general
Astrophysics - Cosmology and Nongalactic Astrophysics
Subjects
Details
- Language :
- English
- ISSN :
- 95500510 and 00358711
- Database :
- OpenAIRE
- Journal :
- arXiv, Monthly Notices of the Royal Astronomical Society, 460(4), 4320-4347. Oxford University Press, Monthly Notices of the Royal Astronomical Society
- Accession number :
- edsair.doi.dedup.....8aa96169236b35557811872110f22447