We present a measurement of the abundance of carbon monoxide in the early universe,
utilizing the final results from the CO Power Spectrum Survey (COPSS). Between 2013 and …

Line intensity mapping (LIM) is a promising approach to study star formation and the
interstellar medium (ISM) in galaxies by measuring the aggregate line emission from the …

We compile available constraints on the carbon monoxide (CO) 1-0 luminosity functions and
abundances at redshifts 0–3. This is used to develop a data driven halo model for the …

Radio astronomy is a discipline of dynamics and wonders. The vast universe has many
secrets to unravel. As one of the important facilities in this discipline, radio telescopes play a …

Abstract In 2018, the Greenland Telescope (GLT) started scientific observation in Greenland.
Since then, we have completed several significant improvements and added new …

Cosmic microwave background (CMB) experiments that constrain the tensor-to-scalar ratio r
are now approaching the sensitivity at which delensing—removing the B modes induced by …

We present a multiwavelength analysis of a sample of four hot (TX> 8 keV) X-ray galaxy
clusters (A1689, A2261, A2142, and A2390) using joint AMiBA Sunyaev–Zel'dovich effect …

We present constraints on the abundance of carbon monoxide in the early universe from the
CO Power Spectrum Survey. We utilize a data set collected between 2005 and 2008 using …

We consider the potential for line intensity mapping (IM) experiments to measure the baryon
acoustic oscillations (BAO) from 3< z< 6. This would constrain the expansion history in a …

To investigate the dynamics of the galaxy cluster A2142, we compile an extended catalog of
2239 spectroscopic redshifts of sources, including 237 newly measured redshifts, within 30 …