COMAP Early Science: I. Overview

The CO Mapping Array Project (COMAP) aims to use line intensity mapping of carbon monoxide (CO) to trace the distribution and global properties of galaxies over cosmic time, back to the Epoch of Reionization (EoR). To validate the technologies and techniques needed for this goal, a Pathfinder instrument has been constructed and fielded. Sensitive to CO(1-0) emission from \(z=2.4\)-\(3.4\) and a fainter contribution from CO(2-1) at \(z=6\)-8, the Pathfinder is surveying \(12\) deg\(^2\) in a 5-year observing campaign to detect the CO signal from \(z\sim3\). Using data from the first 13 months of observing, we estimate \(P_\mathrm{CO}(k) = -2.7 \pm 1.7 \times 10^4\mu\mathrm{K}^2 \mathrm{Mpc}^3\) on scales \(k=0.051-0.62 \mathrm{Mpc}^{-1}\) - the first direct 3D constraint on the clustering component of the CO(1-0) power spectrum. Based on these observations alone, we obtain a constraint on the amplitude of the clustering component (the squared mean CO line temperature-bias product) of \(\langle Tb\rangle^2