Daniel Schaerer
Published 2014-07-10Version 1
I provide an overview about star-forming galaxies at high redshift and their physical properties. Starting from the populations of Ly-$\alpha$ emitters and Lyman break galaxies, I summarize their common features and distinction. Then I summarize recent insight onto their physical properties gained from SED models including nebular emission, and various implications from these studies on the properties of star-formation at high redshift. Finally, I present new results and an overview on the dust content and UV attenuation of $z>6$ galaxies obtained from IRAM and ALMA observations.
Comments: 12 pages, 5 figures. To appear in "LESSONS FROM THE LOCAL GROUP - A Conference in Honour of David Block and Bruce Elmegreen", eds. Freeman, K.C., Elmegreen, B.G., Block, D.L. & Woolway, M. (SPRINGER: NEW YORK)
A search for Population III galaxies in CLASH. I. Singly-imaged candidates at high redshift
Massive and old quiescent galaxies at high redshift
The IMF from Low to High Redshift
![QR code for arXiv:1407.2796 [astro-ph.GA]](http://oss.arxitics.com/images/favicon.svg)