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First limits on the 21 cm power spectrum during the Epoch of X-ray heating

Authors :
Thiagaraj Prabu
Lincoln J. Greenhill
Jonathan C. Pober
Stephen M. Ord
Andrei Mesinger
Eric Kratzenberg
Nichole Barry
Bartosz Pindor
Han-Seek Kim
Edward H. Morgan
J. L. B. Line
Christopher L. Williams
A. de Oliveira-Costa
Ian Sullivan
Benjamin McKinley
Joshua S. Dillon
David L. Kaplan
Andrew Williams
Daniel A. Mitchell
A. Roshi
N. Udaya Shankar
Cathryn M. Trott
Nithyanandan Thyagarajan
Rachel L. Webster
K. S. Srivani
J. Riding
Judd D. Bowman
Bryna J. Hazelton
Bryan Gaensler
A. R. Offringa
Miguel F. Morales
Lu Feng
Natasha Hurley-Walker
Pietro Procopio
Emil Lenc
Frank H. Briggs
Abraham R. Neben
Mark Waterson
Alan R. Whitney
Adam P. Beardsley
Gianni Bernardi
Chen Wu
Mervyn J. Lynch
Aaron Ewall-Wice
J. S. B. Wyithe
David Emrich
Brian E. Corey
P. Carroll
Justin C. Kasper
Max Tegmark
Shiv K. Sethi
Melanie Johnston-Hollitt
Divya Oberoi
Ravi Subrahmanyan
S. Paul
Randall B. Wayth
Abraham Loeb
Robert F. Goeke
Steven Tingay
Alan E. E. Rogers
Daniel C. Jacobs
Jacqueline N. Hewitt
Colin J. Lonsdale
Roger J. Cappallo
Stephen R. McWhirter
Massachusetts Institute of Technology. Department of Physics
MIT Kavli Institute for Astrophysics and Space Research
Ewall-Wice, Aaron Michael
Dillon, Joshua Shane
Hewitt, Jacqueline N
Neben, Abraham Richard
Tegmark, Max Erik
Feng, Lu
Goeke, Robert F
Astronomy
Ewall-Wice, A.
Dillon, Joshua S.
Hewitt, J. N.
Loeb, A.
Mesinger, A.
Neben, A. R.
Offringa, A. R.
Tegmark, M.
Barry, N.
Beardsley, A. P.
Bernardi, G.
Bowman, Judd D.
Briggs, F.
Cappallo, R. J.
Carroll, P.
Corey, B. E.
de Oliveira-Costa, A.
Emrich, D.
Feng, L.
Gaensler, B. M.
Goeke, R.
Greenhill, L. J.
Hazelton, B. J.
Hurley-Walker, N.
Johnston-Hollitt, M.
Jacobs, Daniel C.
Kaplan, D. L.
Kasper, J. C.
Kim, H
Kratzenberg, E.
Lenc, E.
Line, J.
Lonsdale, C. J.
Lynch, M. J.
Mckinley, B.
Mcwhirter, S. R.
Mitchell, D. A.
Morales, M. F.
Morgan, E.
Thyagarajan, Nithyanandan
Oberoi, D.
Ord, S. M.
Sourabh, Paul
Pindor, B.
Pober, J. C.
Prabu, T.
Procopio, P.
Riding, J.
Rogers, A. E. E.
Roshi, A.
Shankar, N. Udaya
Sethi, Shiv K.
Srivani, K. S.
Subrahmanyan, R.
Sullivan, I. S.
Tingay, S. J.
Trott, C. M.
Waterson, M.
Wayth, R. B.
Webster, R. L.
Whitney, A. R.
Wu, C.
Wyithe, J. S. B.
Mesinger, ANDREI ALBERT
ITA
USA
AUS
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)

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