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Galaxy Growth at Early Times from 3D Studies

Published online by Cambridge University Press:  09 February 2015

N. M. Förster Schreiber  and
the SINS/zC-SINF & KMOS3D teams
N. M. Förster Schreiber
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany email: forster@mpe.mpg.de
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Abstract

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Spatially- and spectrally-resolved studies have proven very powerful in exploring the processes driving baryonic mass assembly and star formation at redshifts z ∼ 1–3, the heyday of massive galaxy formation. This contribution presents selected key results from near-infrared integral field spectroscopic studies of z ∼ 1–3 galaxies, including from the SINS/zC-SINF and KMOS3D surveys with SINFONI and KMOS at the ESO Very Large Telescope, highlights synergies with observations at other wavelengths, and discusses some of the implications for early galaxy evolution from mass assembly to feedback processes.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 232 - 238
Copyright
Copyright © International Astronomical Union 2015 

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