Sensitivity for 21 cm bispectrum from Epoch of Reionization
نویسندگان
چکیده
منابع مشابه
Improving Foreground Subtraction in Statistical Observations of 21 Cm Emission from the Epoch of Reionization
Statistical observations of the Epoch of Reionization using the 21 cm line of neutral hydrogen have the potential to revolutionize our understanding of structure formation and the first luminous objects. However, these observations are complicated by a host of strong foreground sources. Several foreground removal techniques have been proposed in the literature, and it has been assumed that thes...
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The redshifted 21-cm line of distant neutral H atoms provides a probe of the cosmic “dark ages” and the epoch of reionization (“EOR”) which ended them, within the first billion years of cosmic time. The radio continuum produced by this redshifted line can be seen in absorption or emission against the cosmic microwave background (“CMB”) at meterwaves, yielding information about the thermal and i...
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We investigate the 21-cm emission from the epoch between reionization zr and Gunn-Peterson transparency zgp. According to the lognormal model of the thermal history around reionization, hydrogen clouds in zr > z > zgp are hot, and a predominant part of baryonic gas is ionized, but still opaque to Lyα photons. Therefore, 21-cm emission is a distinctive characteristic of this epoch. We show that ...
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During the epoch of reionization, Ly-α photons emitted by the first stars can couple the neutral hydrogen spin temperature to the kinetic gas temperature, providing the opportunity to observe the gas in emission or absorption in the 21-cm line. Given the bright foregrounds, it is of prime importance to determine precisely the fluctuations signature of the signal, to be able to extract it by its...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2015
ISSN: 1365-2966,0035-8711
DOI: 10.1093/mnras/stv855