COMAP Home Science Instrument Team News Publications Internal Contact C O M A P The CO Mapping Array PROJECT line intensity mapping with carbon monoxide  What is COMAP? The CO Mapping Array Project (COMAP) is part of a program aiming to trace the spatial distribution of star-forming galaxies at the Epoch of Reionization (EoR). Constraining the CO power spectrum from the EoR will ultimately require measurements at multiple frequencies and focal-plane arrays with hundreds of elements. As a first step towards this goal, COMAP: Pathfinder comprises a 10.4-m telescope, located at the Owens Valley Radio Observatory (OVRO), equipped with a 19-pixel spectrometer array that is mapping a total of around 12 square degrees of sky in the frequency range 26-34 GHz, with spectral resolution R~800. This band is sensitive to CO(1-0) in the redshift slice z=2.4-3.4 and to CO(2-1) in the redshift slice z = 5.8-7.8. A CASPER-based digital backend is used to process 8 GHz from each of the 19 pixels. The aim of this Pathfinder is to i) demonstrate the feasibility and future potential of wide-field CO intensity mapping, and ii) provide a test-bed for the technology development and observational strategies. The science focus of the Pathfinder is on detecting the CO power spectrum and deriving constraints on the global properties of galaxies at z=2.4-3.4. The next stage of the experiment, COMAP:EoR, will provide constraints on galaxies through the end of the Epoch of reionization, at z=4.5-8, as well as adding sensitivity at z=2-3. November 2024: Season 2 Results Published! Learn More July 2022: Early Science papers published! Learn More Latest COMAP Collaboration Publications Lunde+2024: "COMAP Pathfinder – Season 2 results I. Improved data selection and processing" Stutzer+2024: "COMAP Pathfinder – Season 2 results II. Updated constraints on the CO(1–0) power spectrum" Chung+2024: "COMAP Pathfinder – Season 2 results III. Implications for cosmic molecular gas content at z ~ 3" Dunne+ 2024: "COMAP Early Science. VIII. A Joint Stacking Analysis with eBOSS Quasars" COMAP Science & Instrument Science Although the ultimate goal of COMAP is to target the EoR, Phase I will focus on the lower redshifts accessible to a Pathfinder-scale experiment: z = 2.4 - 3.4, at the peak of the cosmic star-formation rate density, during the Epoch of Galaxy Assembly. Learn More Instrument COMAP Phase I is a single-dish experiment, using a 19-feed focal plane array operating at 26-34 GHz, deployed on a 10.4-m telescope at the Owens Valley Radio Observatory. Learn More This material is based upon work supported by the National Science Foundation under Grant Numbers AST 1517108, 1517288, 1517598, 1518282, 1910999 and 2206834, and by the Keck Institute for Space Studies under "The First Billion Years: A Technical Development Program for Spectral Line Observations." Parts of the work were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration, and funded through the internal Research and Technology Development program. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.