Speaker
Phil Bull
(Jodrell Bank Centre for Astrophysics)
Description
I briefly review the instrument specifications that would be necessary to support a 21cm intensity mapping science case with ARGOS. The upshot is that a dense core would be needed, either with lower frequency receivers on 6m dishes, or the proposed L-band receivers on 3m dishes. Control of systematics such as mutual coupling is paramount, and basic pointing capability would be desirable to increase the accessible survey area.
Author
Phil Bull
(Jodrell Bank Centre for Astrophysics)
