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Symposium 241
Symposium 241
Abstract details
The stellar population in the high redshift universe
D.Schaerer, A.Hempel, R.Pell\'o, E.Egami, J.Richard, J.P.Kneib, M.WiseAbstract
We present new results following up on our deep near-IR imagingof the strong lensing clusters Abell 1835 and AC114, which has allowed us to identify 13 star forming galaxy candidates at $z \ga$ 7 (Richard et al.\ 2006, A\&A in press, [astro-ph/0606134]).
Our previous optical and near-IR observations have now been complemented by new deep imaging with ACS/HST in the z$_{850}$ band, with Spitzer IRAC and MIPS at longer wavelengths, and with new Chandra observations.The ACS images confirm all of our high-$z$ candidates as optical
drop-out sources.
Based on these new data we will present a re-analysis of our
high-$z$ candidates and the constraints on the star formation
history at $z \sim$ 6--10.
Based on detailed SED modeling, using spectral templates of Bruzual \& Charlot, Schaerer(starburst), Maraston (including TP-AGB stars) and others, we will quantify their photometric
redshifts, compare them with our spectroscopic observations,
and we will discuss the properties of the individual objects.