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arXiv · 1905.06927

Early Low-Mass Galaxies and Star-Cluster Candidates at z~6-9 Identified by the Gravitational Lensing Technique and Deep Optical/Near-Infrared Imaging

Shotaro Kikuchihara·Masami Ouchi·Yoshiaki Ono·Ken Mawatari·Jacopo Chevallard·Yuichi Harikane·Takashi Kojima·Masamune Oguri·Gustavo Bruzual·Stephane Charlot
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Abstract

We present very faint dropout galaxies at z~6-9 with a stellar mass M* down to M*~10^6Mo that are found in deep optical/near-infrared (NIR) images of the full data sets of the Hubble Frontier Fields (HFF) program in conjunction with deep ground-based and Spitzer images and gravitational lensing magnification effects. We investigate stellar populations of the HFF dropout galaxies with the optical/NIR photometry and BEAGLE models made of self-consistent stellar population synthesis and photoionization models, carefully including strong nebular emission impacting on the photometry. We identify 357 galaxies with M*~10^6-10^9Mo, and find that a stellar mass to UV luminosity L_UV ratio M*/L_UV is nearly constant at M*~10^6-10^9Mo. Our best-estimate M*/L_UV function is comparable to a model of star-formation duration time of 100 Myr, but 2-7 times higher than the one of 10 Myr assumed in a previous study (at the 5sigma level) that would probably underestimate M* of faint galaxies. We derive the galaxy stellar mass functions (GSMFs) at z~6-9 that agree with those obtained by previous studies with no M*/L_UV assumptions at M*>~10^8Mo, and that extends to M*~10^6Mo. Estimating the stellar mass densities rho* with the GSMFs, we find that rho* smoothly increases from log(rho*/[Mo Mpc^(-3)])=5.91 +0.75/-0.65 at z~9 to 6.21 +0.39/-0.37 at z~6-7, which is consistent with the one estimated from star-formation rate density measurements. In conjunction with the estimates of the galaxy effective radii R_e on the source plane, we have pinpointed two objects with low stellar masses (M*<=10^7Mo) and very compact morphologies (R_e<=40 physical pc) that are comparable with those of globular clusters (GCs) in the Milky Way today. These objects are candidates of star clusters that should be a part or a dominant component of high-redshift low-mass galaxy, some of which may be related to GCs today.

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Shotaro Kikuchihara, Masami Ouchi, Yoshiaki Ono, Ken Mawatari, Jacopo Chevallard, Yuichi Harikane, Takashi Kojima, Masamune Oguri, Gustavo Bruzual, Stephane Charlot. 2019-05-16. Early Low-Mass Galaxies and Star-Cluster Candidates at z~6-9 Identified by the Gravitational Lensing Technique and Deep Optical/Near-Infrared Imaging. https://doi.org/10.3847/1538-4357%2Fab7dbe

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