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The first power spectrum limit on the 21-cm signal of neutral hydrogen during the Cosmic Dawn at z=20-25 from LOFAR

Gehlot, B. K. (author)
Mertens, F. G. (author)
Koopmans, L. V. E. (author)
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Brentjens, M. A. (author)
Zaroubi, S. (author)
Ciardi, B. (author)
Ghosh, A. (author)
Hatef, M. (author)
Iliev, I. T. (author)
Jelić, V. (author)
Kooistra, R. (author)
Krause, F. (author)
Mellema, Garrelt (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Mevius, M. (author)
Mitra, M. (author)
Offringa, A. R. (author)
Pandey, V. N. (author)
Sardarabadi, A. M. (author)
Schaye, J. (author)
Silva, M. B. (author)
Vedantham, H. K. (author)
Yatawatta, S. (author)
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 (creator_code:org_t)
2019-07-12
2019
English.
In: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 488:3, s. 4271-4287
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Observations of the redshifted 21-cm hyperfine line of neutral hydrogen from early phases of the Universe such as Cosmic Dawn and the Epoch of Reionization promise to open a new window onto the early formation of stars and galaxies. We present the first upper limits on the power spectrum of redshifted 21-cm brightness temperature fluctuations in the redshift range z = 19.8-25.2 (54-68 MHz frequency range) using 14 h of data obtained with the LOFAR-Low Band Antenna (LBA) array. We also demonstrate the application of a multiple pointing calibration technique to calibrate the LOFAR-LBA dual-pointing observations centred on the North Celestial Pole and the radio galaxy 3C220.3, We observe an unexplained excess of similar to 30-50 per cent in Stokes / noise compared to Stokes V for the two observed fields, which decorrelates on greater than or similar to 12 s and might have a physical origin. We show that enforcing smoothness of gain errors along frequency direction during calibration reduces the additional variance in Stokes I compared Stokes V introduced by the calibration on sub-band level. After subtraction of smooth foregrounds, we achieve a 2 sigma upper limit on the 21-cm power spectrum of Delta(2)(21) < (14561 mK)(2) at k similar to 0.038 h cMpc(-1) and Delta(2)(21) < (14886 mK)(2) at k 0.038 h cMpc(-1) for the 3C220 and NCP fields respectively and both upper limits are consistent with each other. The upper limits for the two fields are still dominated by systematics on most k modes.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

methods: data analysis
methods: statistical
techniques: interferometric
dark ages
reionization
first stars
diffuse radiation
radio lines: general

Publication and Content Type

ref (subject category)
art (subject category)

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