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- W3105223883 abstract "We obtained mid-infrared 3.6 and 4.5|$ mu$|m imaging of a |$z =$| 6.96 Ly|$alpha $| emitter (LAE), IOK-1, discovered in the Subaru Deep Field, using Spitzer Space Telescope Infrared Array Camera observations. After removal of a nearby bright source, we found that IOK-1 is not significantly detected in any of these infrared bands to |$m_{3.6mu{rm m}} sim$| 24.00 and |$m_{4.5mu{rm m}} sim$| 23.54 at 3|$ sigma$|. Fitting population synthesis models to the spectral energy distribution consisting of the upper limit fluxes of the optical-to-infrared non-detection images and fluxes in detection images, we constrained the stellar mass, |$M_ast$|, of IOK-1. This LAE could have either a mass as low as |$M_ast lesssim$| 2–9 |$times$| 10|$^{8} M_{odot}$| for young age (|$lesssim$|10 Myr) and low dust reddening (|$A_V sim$| 0) or a mass as large as |$M_ast lesssim$| 1–4 |$times$| 10|$^{10} M_{odot}$| for either old age (|$ gt $|100 Myr) or high dust reddening (|$A_V sim$| 1.5). This would be within the range of masses of |$z sim$| 3–6.6 LAEs studied to date, |$sim$|10|$^6$|–10|$^{10} M_{odot}$|. Hence, IOK-1 is not a particularly unique galaxy with extremely high mass or low mass, but is similar to one of the LAEs seen at later epochs." @default.
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- W3105223883 date "2010-10-25" @default.
- W3105223883 modified "2023-10-16" @default.
- W3105223883 title "Spitzer Space Telescope Constraint on the Stellar Mass of a<i>z</i>= 6.96 Lyα Emitter" @default.
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- W3105223883 doi "https://doi.org/10.1093/pasj/62.5.1167" @default.
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