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Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
Square Kilometre Array Cosmology Science Working Group, David J. Bacon, Richard A. Battye +44
We present a detailed overview of the cosmological surveys that will be carried out with Phase 1 of the Square Kilometre Array (SKA1), and the science that they will enable. We hig…
Constraining the evolution of CII intensity through the end stages of reionization
Hamsa Padmanabhan
We combine available constraints on the local CII 158 m line luminosity function from galaxy observations (Hemmati et al. 2017), with the evolution of the star-formation rate de…
Fundamental Physics with the Square Kilometre Array
A. Weltman, P. Bull, S. Camera +50
The Square Kilometre Array (SKA) is a planned large radio interferometer designed to operate over a wide range of frequencies, and with an order of magnitude greater sensitivity an…
Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy Surveys
Dongwoo T. Chung, Marco P. Viero, Sarah E. Church +15
Line-intensity mapping (LIM or IM) is an emerging field of observational work, with strong potential to fit into a larger effort to probe large-scale structure and small-scale astr…
Joint power spectrum and voxel intensity distribution forecast on the CO luminosity function with COMAP
Håvard Tveit Ihle, Dongwoo Chung, George Stein +12
We develop a framework for joint constraints on the CO luminosity function based on power spectra (PS) and voxel intensity distributions (VID), and apply this to simulations of COM…
Impact of astrophysics on cosmology forecasts for 21 cm surveys
Hamsa Padmanabhan, Alexandre Refregier, Adam Amara
We use the results of previous work building a halo model formalism for the distribution of neutral hydrogen, along with experimental parameters of future radio facilities, to plac…