Orateur
Kieran Cleary
(California Institute of Technology)
Description
Carbon monoxide is one of the main targets for line intensity mapping, offering the potential to trace the dense gas history of the universe during the Epoch of Galaxy Assembly, and the galactic sources of ionization at the Epoch of Reionization. We review the features of CO emission that make it attractive for this purpose, discuss the current and future experimental landscape and in particular, describe the current status and next phases of the CO Mapping Array Project.
Author
Kieran Cleary
(California Institute of Technology)
