arXiv · 1903.01884
The UV and Ly$\alpha$ Luminosity Functions of galaxies and the Star Formation Rate Density at the end of HI reionization from the VIMOS Ultra-Deep Survey (VUDS)
Abstract
We establish a robust statistical description of the star-forming galaxy population at the end of cosmic HI reionization ($5.0\le{}z\le6.6$) from a large sample of 52 galaxies with spectroscopically confirmed redshifts from the VIMOS UltraDeep Survey. We identify galaxies with Ly$\alpha$ either in absorption or in emission, at variance with most spectroscopic samples in the literature where Ly$\alpha$ emitters dominate. We find that star-forming galaxies at these redshifts are distributed along a main sequence in the stellar mass vs. SFR plane. We report a flat evolution of the sSFR(z) in 3 2. The bright end of the Ly$\alpha$ luminosity function has a high number density, indicating a significant star formation activity concentrated in the brightest Ly$\alpha$ emitters (LAE) at these redshifts. LAE with EW>25\AA ~contribute to about 75\% of the total UV-derived SFRD. While our analysis favors a low dust content in 5.0<z<6.6, uncertainties on the dust extinction correction and associated degeneracies in spectral fitting will remain an issue to estimate the total SFRD until future survey extending spectroscopy to the NIR rest-frame spectral domain, e.g. with JWST.
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Y. Khusanova, O. Le Fèvre, P. Cassata, O. Cucciati, B. C. Lemaux, L. A. M. Tasca, R. Thomas, B. Garilli, V. Le Brun, D. Maccagni, L. Pentericci, G. Zamorani, R. Amorín, S. Bardelli, M. Castellano, L. P. Cassarà, A. Cimatti, M. Giavalisco, N. P. Hathi, O. Ilbert, A. M. Koekemoer, F. Marchi, J. Pforr, B. Ribeiro, D. Schaerer, L. Tresse, D. Vergani, E. Zucca. 2019-03-05. The UV and Ly$\alpha$ Luminosity Functions of galaxies and the Star Formation Rate Density at the end of HI reionization from the VIMOS Ultra-Deep Survey (VUDS). https://doi.org/10.1051/0004-6361%2F201935400
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