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I provide an overview about star-forming galaxies at high redshift and theirphysical properties. Starting from the populations of Ly-$\alpha$ emitters andLyman break galaxies, I summarize their common features and distinction. Then Isummarize recent insight onto their physical properties gained from SED modelsincluding nebular emission, and various implications from these studies on theproperties of star-formation at high redshift. Finally, I present new resultsand an overview on the dust content and UV attenuation of $z>6$ galaxiesobtained from IRAM and ALMA observations.

Lyman alpha emitting and related star-forming galaxies at high redshift