Slide 1The Far-Infrared Universe: from the Universe’s oldest light to the birth of its youngest stars Jeremy P. Scott, on behalf of Locke D. Spencer Physics and Astronomy,…

Slide 1 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) The Gunn Peterson Effect Fan et al 2003 Fast…

VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/FTIR Similar gas properties in arm and interarm regions. Higher densities and stronger radiation fields…

History of IGM bench-mark in cosmic structure formation indicating the first luminous structures Epoch of Reionization (EoR) C.Carilli (NRAO) CfA Sept 2004 ionized neutral…

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 host galaxies at z…

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 host galaxies at z…

History of IGM last phase of cosmic evolution to be tested bench-mark in cosmic structure formation indicating the first luminous structures Epoch of Reionization (EoR) C.Carilli…

Radio astronomical probes of Cosmic Reionization and the 1st luminous objects Chris Carilli March 19, 2007 University of Colorado Brief introduction to cosmic reionization…

History of IGM bench-mark in cosmic structure formation indicating the first luminous structures Epoch of Reionization (EoR) The Gunn Peterson Effect Fan et al 2003 Fast…