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- W2108182983 abstract "Three-dimensional panchromatic dust radiative transfer calculations are performed on a set of 198 galaxies of stellar masses in the range 5x10^8-3x10^10 Msun from a cosmological hydrodynamic simulation (resolved at 29pc/h) at z=7. In a companion paper (Kimm & Cen), the stellar mass and UV luminosity functions, and UV-optical and FUV-NUV colors are shown to be in good agreement with observations, if an SMC-type dust extinction curve is adopted. Here we make useful predictions, self-consistently, of the infrared properties of these z=7 simulated galaxies that can be confronted with upcoming ALMA data. Our findings are as follows. (1) The effective radius in the rest-frame MIPS 70 micron band is in the range of 80-400pc proper for z=7 galaxies with L_FIR=10^{11.3-12}Lsun. (2) The median of the peak wavelength of the far-infrared (FIR) spectral energy distribution is in the range of 45-60 micron, depending on the dust-to-metal ratio. (3) For star formation rate in the range 3-100 Msun/yr the median FIR to bolometric luminosity ratio is 60-90%. (4) The FIR luminosity function displays a power law in the high end with a slope of -3.1 +- 0.4, instead of the usual exponential decline." @default.
- W2108182983 created "2016-06-24" @default.
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- W2108182983 date "2014-01-23" @default.
- W2108182983 modified "2023-09-23" @default.
- W2108182983 title "INFRARED PROPERTIES OFz= 7 GALAXIES FROM COSMOLOGICAL SIMULATIONS" @default.
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- W2108182983 doi "https://doi.org/10.1088/0004-637x/782/1/32" @default.
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