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IGM and CGM Emission Mapping: A New Window on Galaxy and Structure Formation

Published onMay 31, 2019
IGM and CGM Emission Mapping: A New Window on Galaxy and Structure Formation
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Abstract

We describe the prospects for IGM and CGM emission mapping with UV resonance lines at low and high redshift. There are 5 key science questions that will be addressed: 1) A Lyman alpha emission calibration; 2) physical properties of galaxy halos; 3) the role and nature of gas inflows to galaxies; 4) gas outflows: 5) emission from the cosmic web.

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