“From the Very First Stars to z~6 Galaxies and Quasars”

Dr. Michele Trenti
STScI
High redshift observations are opening larger and larger windows on galaxy formation and evolution in the first billion years of the Universe, with very rare bright quasars identified from all-sky surveys and more common galaxies observed through deep narrow-beam programs, such as GOODS and the UDF. Using cosmological simulations of structure formation I will first quantify the typical systematic uncertainties in the observed luminosity function due to cosmic variance, not only in its normalization but also in the shape. I will then discuss the link between these z~6 galaxies and quasars and the very first "Pop III" stars formed at z>40, which provide early seeding for supermassive black hole growth.