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The Large Millimeter Telescope - Berkeley Center for Cosmological ...

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Cosmology at millimeter-wavelengths<br />

• can detect the earliest evolutionary stages of structure<br />

<strong>for</strong>mation in planet-<strong>for</strong>ming and star-<strong>for</strong>ming regions<br />

(cold, dense, optically-thick dust-obscured environments)<br />

• independence of flux density on distance means we can<br />

detect starburst galaxies in the high-z Universe (which contribute<br />

~50% of the γ-ray to radio extragalactic background light)<br />

• rich molecular-line spectrum to understand physical<br />

conditions of star<strong>for</strong>mation, the ISM, gas mass,<br />

spectroscopic–z & evolutionary history<br />

• we observe the CMB at the peak of its energy distribution.<br />

Sunyaev-Zeldovich effect is a powerful redshift-independent<br />

method to identify clusters in local and high-z Universe

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