Predictions for measuring the cross power spectrum of the HI 21-cm signal and the Lyman-α forest using OWFA
Author:
Publisher
IOP Publishing
Subject
Astronomy and Astrophysics
Link
http://stacks.iop.org/1475-7516/2018/i=05/a=051/pdf
Reference63 articles.
1. The IUE Survey for Damped Lyman- alpha and Lyman-Limit Absorption Systems: Evolution of the Gaseous Content of the Universe
2. The ESO UVES advanced data products quasar sample
3. Using HI to probe large scale structures at z∼3
4. HI fluctuations at large redshifts: I-visibility correlation
5. Possibility of Precise Measurement of the Cosmological Power Spectrum with a Dedicated Survey of 21 cm Emission after Reionization
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2. Constraining dark energy using the cross correlations of weak lensing with post-reionization probes of neutral hydrogen;Journal of Cosmology and Astroparticle Physics;2021-02-09
3. Simulated predictions for H i at z = 3.35 with the Ooty Wide Field Array (OWFA) – II. Foreground avoidance;Monthly Notices of the Royal Astronomical Society;2020-10-29
4. Constraining warm dark matter power spectrum using the cross-correlation of HI 21 cm signal and the Lyman-α forest;Journal of Cosmology and Astroparticle Physics;2019-12-19
5. Modelling the post-reionization neutral hydrogen (H i) 21-cm bispectrum;Monthly Notices of the Royal Astronomical Society;2019-10-10
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