The 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.
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)
VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/F TIR Similar gas properties in arm and interarm regions. Higher densities and stronger.
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
Studying the gas, dust, and star formation in the first galaxies at cm and mm wavelengths
Radio astronomical probes of Cosmic Reionization and the 1 st luminous objects
Massive galaxy (and black hole) formation in the early Universe Chris Carilli (NRAO) Berkeley, February 10, 2009 Intro: telescopes, techniques, massive.
![VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/F TIR Similar gas properties in arm and interarm regions. Higher densities and stronger.](https://static.fdocuments.in/doc/330x215/56649edb5503460f94bea5fd/vngs-science-highlight-pdr-models-of-m51-ciioi63-ciioi63f-tir.jpg)
