Survey parameters for detecting 21-cm-Ly α emitter cross-correlations with the Square Kilometre Array. (22nd June 2018)

• Record Type: Journal Article
• Authors: Hutter, Anne; Trott, Cathryn M; Dayal, Pratika
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 479:Number 1(2018:Sep.)
• Page Start: L129
• Page End: L133
• Publication Date: 2018-06-22
• Subjects: radiative transfer -- methods: numerical -- galaxies: high-redshift -- galaxies: intergalactic medium -- cosmology: dark ages, reionization, first stars; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/sly115
• Languages: English
• ISSNs: 1745-3933

Abstract

Abstract: Detections of the cross-correlation signal between the 21 cm signal during reionization and high-redshift Lyman-α (Ly α) emitters (LAEs) are subject to observational uncertainties which mainly include systematics associated with radio interferometers and LAE selection. These uncertainties can be reduced by increasing the survey volume and/or the survey luminosity limit, i.e. the faintest detectable Ly α luminosity. We use our model of high-redshift LAEs and the underlying reionization state to compute the uncertainties of the 21-cm-LAE cross-correlation function at $z$ ≃ 6.6 for observations with SKA1-Low and LAE surveys with Δ$z$ = 0.1 for three different values of the average inter-galactic medium (IGM) ionization state (⟨χH i ⟩ ≃ 0.1, 0.25, 0.5). At $z$ ≃ 6.6, we find SILVERRUSH type surveys, with a field of view of 21 deg 2 and survey luminosity limits of L α ≥ 7.9 × 10 42 erg s −1, to be optimal to distinguish between an IGM that is 50 , 25 , and 10 per cent neutral, while surveys with smaller fields of view and lower survey luminosity limits, such as the 5 and 10 deg 2 surveys with WFIRST, can only discriminate between a 50 and 10 per cent neutral IGM.