Insights into Galaxy Evolution from Mid-infrared Wavelengths - INSPIRE

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Insights into Galaxy Evolution from Mid-infrared Wavelengths

Ranga-Ram Chary
(
- Spitzer Space Telescope
)

Dec, 2006

11 pages

Published in:

ASP Conf.Ser. 380 (2007) 375

Contribution to:

At the Edge of the Universe: Latest Results from the Deepest Astronomical Surveys, 375

e-Print:

astro-ph/0612736 [astro-ph]

View in:

ADS Abstract Service

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Abstract: (arXiv)

In this paper, I have attempted to highlight key results from deep extragalactic surveys at mid-infrared wavelengths. I discuss advances in our understanding of dust enshrouded star-formation and AGN activity at 03 will become possible only with future facilities like ALMA. Currently, the presence of dust can only be assessed in a small fraction of the youngest starbursts at z>5 by looking for redshifted large equivalent width H_alpha emission in broadband filters like the IRAC 4.5 micron passband. H_alpha to UV ratios in these objects are a tracer of dust extinction and measuring this ratio in GOODS galaxies indicate dust in ~20% of star-forming galaxies at z>5. Finally, implications for reionization based on the measured stellar mass density and star-formation rates of galaxies at these redshifts are discussed.

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