Until now, investigating the early stages of galaxy formation has been primarily the realm of theoretical modeling and computer simulations, which require many physical ingredients and are challenging to test observationally. However, the latest Hubble Space Telescope observations in the near infrared are shedding new light on the properties of galaxies within the first billion years after the Big Bang, including our recent discovery of the most distant proto-cluster of galaxies at redshift z ∼ 8. Here, I compare predictions from models of primordial and metal-enriched star formation during the dark ages with the latest Hubble observations of galaxies during the epoch of reionization. I focus in particular on the luminosity function and on galaxy clustering as measured from our Hubble Space Telescope Brightest of Reionizing Galaxies (BoRG) survey. BoRG has the largest area coverage to find luminous and rare z ∼ 8 sources that are among the first galaxies to have formed in the Universe.
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12 September 2012
FIRST STARS IV – FROM HAYASHI TO THE FUTURE –
21–25 May 2012
Kyoto, Japan
Research Article|
September 12 2012
The brightest of reionizing galaxies (BoRG) survey
Michele Trenti
Michele Trenti
Kavli Fellow, Institute of Astronomy and Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA,
United Kingdom
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AIP Conf. Proc. 1480, 238–243 (2012)
Citation
Michele Trenti; The brightest of reionizing galaxies (BoRG) survey. AIP Conf. Proc. 12 September 2012; 1480 (1): 238–243. https://doi.org/10.1063/1.4754361
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