Dongwoo Chung

TL;DR: In this paper, the authors report on the recent advances in theory, instrumentation and observation that were presented in these workshops and some of the opportunities and challenges that were identified looking forward.

TL;DR: In this article, the authors present an overview of the motivation and design of Prime-Cam, a first-light instrument for CCAT-prime, a 6-meter aperture telescope operating from sub-mm to mm wavelengths, located at 5600 meters elevation on Cerro Chajnantor in Chile.

TL;DR: The first light instrument for CCAT-prime, Prime-Cam, consists of a 1.8m-diameter cryostat that can house seven individual instrument modules, optimized for a specific science goal, will use state-of-the-art kinetic inductance detector (KID) arrays operated at $${\sim }\,100$$ mK and Fabry-Perot interferometers (FPI) for the epoch of reionization (EoR) science.

TL;DR: In this article, a joint analysis of power spectra and voxel intensity distributions is proposed to constrain the CO luminosity function, which is based on a Markov chain Monte Carlo (MCMCMC) sampler coupled with a Gaussian likelihood.

TL;DR: CCAT-prime as discussed by the authors is a new 6 m crossed Dragone telescope designed to characterize the CMB polarization and foregrounds, measure the Sunyaev-Zel'dovich effects of galaxy clusters, map the [CII] emission intensity from the Epoch of Reionization (EoR), and monitor accretion luminosity over multi-year timescales of hundreds of protostars in the Milky Way.