Deep Spitzer/IRAC Data for z~10 galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ~500 Myr of Cosmic Time
arXiv:2206.13525 · doi:10.3847/1538-4357/aca470
Abstract
We present the deepest constraints yet on the median rest-UV+optical SED of galaxies, prior to JWST science operations. We constructed stacks based on four robust -dropouts, previously identified across the GOODS fields. We used archival HST/WFC3 data and the full depth Spitzer/IRAC mosaics from the GREATS program, the deepest coverage at m to date. The most remarkable feature of the SED is a blue IRAC mag color. We also find a nearly flat mag color, corresponding to a UV slope . This is consistent with previous studies, and indicative of minimal dust absorption. The observed blue IRAC color and SED fitting suggest that galaxies have very young (few Myr) stellar populations, with of stars being formed in the last Myr (). While an exciting result, the uncertainties on the SED are too large to allow us to place strong constraints on the presence of a nebular continuum in galaxies (as might be suggested by the blue mag color). The resulting sSFR is consistent with the specific accretion rate of dark matter halos, indicative of a star-formation efficiency showing quite limited evolution at such early epochs.
Submitted to ApJ. 9 pages, 3 figures. Comments welcome
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