Studying galaxy evolution from reionization to cosmic noon with the latest-generation multiwavelength facilities
In recent years, an array of new ground and space-based observatories operating across the electromagnetic spectrum (e.g. VLT MUSE/KMOS, Subaru/HSC, ALMA, MeerKAT) has transformed our view of star-formation in galaxies through cosmic time, while forthcoming facilities (e.g E-ELT, Euclid, JWST and SKA) will allow the ISM, star-formation and dynamics of galaxies from low to high-redshift to be studied in unprecedented detail. In this session we will explore the panchromatic picture of galaxy evolution, from the peak of star-formation at z~1-3 to the Epoch of Reionization, and consider future prospects for sensitive, high-resolution studies with new facilities in the next decade.
A. Thomson, B. Gullberg, D. Maltby, A. Tiley, J. Wardlow
Wednesday PM1; Thursday AM; Thursday PM1
Faraday LT
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