Future Possibilities for Observing HI at High Redshift
arXiv:astro-ph/9512068 · doi:10.1007/978-94-009-1726-2_53
Abstract
We briefly review the beginnings of HI astronomy, proceed to an assessment of our current capabilities in this area, and continue by considering what will be necessary to push back the frontier to cosmological distances. We then consider how such a leap in performance might be realized.
8 page LaTeX requires crckapb.sty and psfig.sty, 9 compressed and tarred postscript figures (750kB) available at ftp://ftp.nfra.nl/pub/outgoing/rbraun/futposhi/figs.tar.Z Complete compressed postscript paper (790kB) available at ftp://ftp.nfra.nl/pub/outgoing/rbraun/futposhi/paper.ps.Z To appear in "Cold Gas at High Redshift", Eds. M.Bremer et al. (Kluwer, Dordrecht)