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arXiv · 1309.4774

The FMOS-COSMOS survey of star-forming galaxies at z ~ 1.6. I. Hα-based star formation rates and dust extinction

Abstract

We present the first results from a near-IR spectroscopic survey of the COSMOS field, using the Fiber Multi-Object Spectrograph on the Subaru telescope, designed to characterize the star-forming galaxy population at $1.4<z<1.7$. The high-resolution mode is implemented to detect H$α$ in emission between $1.6{\rm -}1.8 \mathrm{μm}$ with $f_{\rm Hα}\gtrsim4\times10^{-17}$ erg cm$^{-2}$ s$^{-1}$. Here, we specifically focus on 271 sBzK-selected galaxies that yield a H$α$ detection thus providing a redshift and emission line luminosity to establish the relation between star formation rate and stellar mass. With further $J$-band spectroscopy for 89 of these, the level of dust extinction is assessed by measuring the Balmer decrement using co-added spectra. We find that the extinction ($0.6\lesssim A_\mathrm{Hα} \lesssim 2.5$) rises with stellar mass and is elevated at high masses compared to low-redshift galaxies. Using this subset of the spectroscopic sample, we further find that the differential extinction between stellar and nebular emission \hbox{$E_\mathrm{star}(B-V)/E_\mathrm{neb}(B-V)$} is 0.7--0.8, dissimilar to that typically seen at low redshift. After correcting for extinction, we derive an H$α$-based main sequence with a slope ($0.81\pm0.04$) and normalization similar to previous studies at these redshifts.

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D. Kashino, J. D. Silverman, G. Rodighiero, A. Renzini, N. Arimoto, E. Daddi, S. J. Lilly, D. B. Sanders, J. Kartaltepe, H. J. Zahid, T. Nagao, N. Sugiyama, P. Capak, C. M. Carollo, J. Chu, G. Hasinger, O. Ilbert, M. Kajisawa, L. J. Kewley, A. M. Koekemoer, K. Kovač, O. Le Fèvre, D. Masters, H. J. McCracken, M. Onodera, N. Scoville, V. Strazzullo, M. Symeonidis, Y. Taniguchi. 2014-03-25. The FMOS-COSMOS survey of star-forming galaxies at z ~ 1.6. I. Hα-based star formation rates and dust extinction. https://doi.org/10.1088/2041-8205%2F777%2F1%2Fl8

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