Star formation at high redshift (2 < z < 7) Methods for deriving star formation rates UV continuum = ionizing photons (dust obscuration?) Ly = ionizing.
History of IGM bench-mark in cosmic structure formation indicating the first luminous structures Epoch of Reionization (EoR)
Cosmic Reionization Chris Carilli (M/NRAO) Vatican Summer School June 2014 I. Introduction: Cosmic Reionization Concept Cool gas in z > 6 galaxies:
History of IGM
Studying the gas, dust, and star formation in the first galaxies at cm and mm wavelengths Chris Carilli, KIAA-PKU reionization workshop, July 2008 QSO.
Radio astronomical probes of the 1 st galaxies Chris Carilli, Aspen, February 2008
ESO
Studying the gas, dust, and star formation in the first galaxies at cm and mm wavelengths
Giant Clouds and Star Clusters in the Antennae
Radio astronomical probes of Cosmic Reionization and the 1 st luminous objects
