Exploring Observational Parameter Space at Very High Redshifts

Details Exploring Observational Parameter Space at Very High Redshifts Exploring Observational Parameter Space at Very High Redshifts

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1294..196b&link_type=abstract

THE FIRST STARS AND GALAXIES: CHALLENGES FOR THE NEXT DECADE. AIP Conference Proceedings, Volume 1294, pp. 196-201 (2010).

Astronomy and Astrophysics

Astronomy

Redshift, Astronomical Telescopes, Clusters Of Galaxies, Intergalactic Matter, Population Iii Stars, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Astrometric And Interferometric Instruments, Galaxy Clusters, Intergalactic Matter, Quasar Absorption And Emission-Line Systems, Lyman Forest, Population Iii Stars

Scientific paper

The low-background spectral region between OH lines in the near infrared and large-area synoptic surveys are two key regimes in which present and future large ground-based telescopes will excel at seeking first-light sources. We will describe the hunt for high-redshift galaxies from the ground, focusing on near-term surveys planned with 8-10 m telescopes and longer-term possibilities with the next generation of extremely large telescopes. We will also discuss progress on the search for high-redshift supernovae from deep time-domain surveys.

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