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{\bf {\LARGE
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Spectroscopic pilot study in the near infrared of a sample of star-forming galaxies at {\em z} $\sim$ 2
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J. Gallego$^{1}$,
A. S\'{a}nchez de Miguel $^{1}$,
J. Zamorano$^{1}$,
P. G. P\'{e}rez-Gonz\'alez$^{1}$,
N.~Cardiel$^{1}$,
and
G. Barro$^{1}$
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$^{1}$
Universidad Complutense de Madrid, E-28040 Madrid, Spain; alex@astrax.fis.ucm.es
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Near-IR spectroscopy of z$\sim$2 star-forming galaxies
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J. Gallego  et al. 
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\section*{Abstract}{\small
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In this work we present the results of the spectroscopic analysis in
the near-infrared $K$ band of a sample of 12 active star forming
galaxies at $z\sim2$. The sample was selected by using photometric
redshifts, blue colors and large fluxes in the 24 $\mu$m band of
MIPS/Spitzer. To analyze their physical properties we have computed
their sizes, colors, stellar masses, extinctions and other parameters
available in literature and in the ”Rainbow” database.  We compute
H$\alpha$ luminosities and star formation rates for all galaxies at
that redshift. We were able to estimate metallicities from [NII]6584
for a sub sample of the objects. In particular the dependence of the metallicity
with the stellar mass has been studied and compared with the results of other samples of
galaxies at several redshifts. For a fixed mass, the metallicities of
our galaxies are compatible than those similar at the corresponding redshift, following the general trend of lower metallicities for higher redshifts.
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\section*{Acknowledgments}   % Do not delete if you declare acknowledgments
\small
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The authors are members of the Consolider-Ingenio 2010 Program grant CSD2006-00070: First Science with the GTC 
(\href{http://www.iac.es/consolider-ingenio-gtc}{http://www.iac.es/consolider-ingenio-gtc}). Partially funded by the Spanish MICINN under the PNAyA 2009-10368. 

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