DOI:
10.1088/0004-637X/795/2/126
IAA authors:
Molino, A.; Jimenez-Teja, Y.
Authors:
Bouwens, R. J.; Bradley, L.; Zitrin, A.; Coe, D.; Franx, M.; Zheng, W.; Smit, R.; Host, O.; Postman, M.; Moustakas, L.; Labbe, I.; Carrasco, M.; Molino, A.; Donahue, M.; Kelson, D. D.; Meneghetti, M.; Benttez, N.; Lemze, D.; Umetsu, K.; Broadhurst, T.; Moustakas, J.; Rosati, P.; Jouvel, S.; Bartelmann, M.; Ford, H.; Graves, G.; Grillo, C.; Infante, L.; Jimenez-Teja, Y.; Lahav, O.; Maoz, D.; Medezinski, E.; Melchior, P.; Merten, J.; Nonino, M.; Ogaz, S.; Seitz, S.
Abstract:
We utilize a two-color Lyman-break selection criterion to search for z similar to 9-10 galaxies over the first 19 clusters in the CLASH program. A systematic search yields three z similar to 9-10 candidates. While we have already reported the most robust of these candidates, MACS1149-JD, two additional z similar to 9 candidates are also found and have H-160- band magnitudes of similar to 26.2-26.9. A careful assessment of various sources of contamination suggests less than or similar to 1 contaminants for our z similar to 9-10 selection. To determine the implications of these search results for the luminosity function (LF) and star formation rate density at z similar to 9, we introduce a new differential approach to deriving these quantities in lensing fields. Our procedure is to derive the evolution by comparing the number of z similar to 9-10 galaxy candidates found in CLASH with the number of galaxies in a slightly lower-redshift sample (after correcting for the differences in selection volumes), here taken to be z similar to 8. This procedure takes advantage of the fact that the relative volumes available for the z similar to 8 and z similar to 9-10 selections behind lensing clusters are not greatly dependent on the details of the lensing models. We find that the normalization of the UV LF at z similar to 9 is just 0.28(-0.20)(+0.39) x that at z similar to 8, which is similar to 1.4(-0.8)(+3.0) x lower than extrapolating z similar to 4-8 LF results. While consistent with the evolution in the UV LF seen at z similar to 4-8, these results marginally favor a more rapid evolution at z > 8. Compared to similar evolutionary findings from the HUDF, our result is less insensitive to large-scale structure uncertainties, given our many independent sightlines on the high-redshift universe.
URL:
https://ui.adsabs.harvard.edu/#abs/2014ApJ...795..126B/abstract
Keywords:
galaxies: evolution; galaxies: high-redshift