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

Autori
Gehlot, B.K. ; Mertens, F.G. ; Koopmans, L.V.E. ; Brentjens, M.A. ; Zaroubi, S. ; Ciardi, B. ; Ghosh, A. ; Hatef, M. ; Iliev, I. T. ; Jelić, Vibor ; Kooistra, R. ; Krause, F. ; Mellema, G. ; Mevius, M. ; Mitra, M. ; Offringa, A.R. ; Pandey, V.N. ; Sardarabadi, A.M. ; Schaye, J. Silva, M.B. ; Vedantham, H.K. ; Yatawatta, S.

Izvornik
Monthly notices of the Royal Astronomical Society (0035-8711) 488 (2019), 3; 4271-4287

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

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

Sažetak
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 ∼30−50 per cent in Stokes / noise compared to Stokes V for the two observed fields, which decorrelates on ≳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 2σ upper limit on the 21-cm power spectrum of Δ221<(14561mK)2 at k∼0.038hcMpc−1 and Δ221<(14886mK)2 at k∼0.038hcMpc−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.

Izvorni jezik
Engleski

Znanstvena područja
Fizika

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