NAM2019
  • NAM2019
    • Registration
    • Key Dates & Outline Schedule
    • Practical Information
    • Exhibitors
    • Grants & Bursaries
    • Contacts
  • Science
    • Science Programme
    • Parallel Sessions
    • Plenary Talks
    • Community Session
    • Special Lunches
    • Posters
    • Presenter Guidelines
  • Social
    • What's On
    • Welcome Reception
    • RAS Awards Dinner
  • Media
  • Outreach
    • Outreach and Education Day
    • Fringe Event
    • School Visit Day
  • Lancaster
    • Travel
    • Accommodation
    • Childcare
    • Campus Map
    • About Lancaster
    • Code of Conduct
  • NAM2019
    • Registration
    • Key Dates & Outline Schedule
    • Practical Information
    • Exhibitors
    • Grants & Bursaries
    • Contacts
  • Science
    • Science Programme
    • Parallel Sessions
    • Plenary Talks
    • Community Session
    • Special Lunches
    • Posters
    • Presenter Guidelines
  • Social
    • What's On
    • Welcome Reception
    • RAS Awards Dinner
  • Media
  • Outreach
    • Outreach and Education Day
    • Fringe Event
    • School Visit Day
  • Lancaster
    • Travel
    • Accommodation
    • Childcare
    • Campus Map
    • About Lancaster
    • Code of Conduct

Parallel sessions

Sessions

id
date time
2019-02-01 11:50:04
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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