COMAP Early Science. II. Pathfinder Instrument
James W. Lamb, Kieran Cleary, D. P. Woody, Morgan Catha, Dongwoo T. Chung, Joshua Ott Gundersen, Stuart Harper, A. I. Harris, R. W. Hobbs, H. T. Ihle, Jonathon Kocz, T. J. Pearson, Liju Philip, Travis Powell, Lilian Basoalto, J. Richard Bond, Jowita Borowska, Patrick C. Breysse, S. Church, C. Dickinson, Delaney A. Dunne, H. K. Eriksen, Marie Kristine Foss, T. Gaier, Junhan Kim, Charles R. Lawrence, J. G. S. Lunde, Hamsa Padmanabhan, Maren Rasmussen, A. C. S. Readhead, R. Reeves, Thomas J. Rennie, Nils-Ole Stutzer, M. Viero, Duncan J. Watts, I. K. Wehus
Abstract
Abstract Line intensity mapping (LIM) is a new technique for tracing the global properties of galaxies over cosmic time. Detection of the very faint signals from redshifted carbon monoxide (CO), a tracer of star formation, pushes the limits of what is feasible with a total-power instrument. The CO Mapping Project Pathfinder is a first-generation instrument aiming to prove the concept and develop the technology for future experiments, as well as delivering early science products. With 19 receiver channels in a hexagonal focal plane arrangement on a 10.4 m antenna and an instantaneous 26–34 GHz frequency range with 2 MHz resolution, it is ideally suited to measuring CO ( J = 1–0) from z ∼ 3. In this paper we discuss strategies for designing and building the Pathfinder and the challenges that were encountered. The design of the instrument prioritized LIM requirements over those of ancillary science. After a couple of years of operation, the instrument is well understood, and the first year of data is already yielding useful science results. Experience with this Pathfinder will guide the design of the next generations of experiments.