Extragalactic Continuum
This working group is focused on the study of continuum emission from galaxies, AGN and galaxy clusters over Cosmic time, including the evolution of the cosmic star-formation rate out to the epoch of reionization.
Extragalactic Continuum Working Group Introduction
Continuum science with the SKA explores our Universe from the nearest star-forming galaxies to high-redshift clusters of galaxies, examining structure formation and evolution on all scales.
![SWG Banner - Continuum](/sites/default/files/styles/ti_1500/public/2022-05/23403_SWG%20Banner%20-%20Continuum.jpg?itok=DuVQ0WRS)
Working Group Membership
Members of the the Extragalactic Continuum Working group can be found here.
We actively encourage interested researchers to participate in the working group.
Please contact the co-chairs if you are interested in joining the group, with a brief description of your area of research.
The current co-chairs are:
- Catherine Hale (Oxford University, UK), catherine.hale@physics.ox.ac.uk
- Fatemeh Tabatabaei (IPM, Iran and IAC/MPIA/MPIfR), ftaba@ipm.ir
Guidelines on who can join the group can be found here.
The SKAO Project Scientist liaison is Wendy Williams (contact details here).
Previous Chairs
- Mark Sargent (2017-2024)
- Natasha Hurley-Walker (2018-2024)
- Rossella Cassano (2015-2018)
- Minh Huynh (2015-2017)
- Isabella Prandoni (2013-2015)
- Nicholas Seymour (2013-2015)
Dernière modification le 26 June 2024