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- W4205697798 endingPage "5578" @default.
- W4205697798 startingPage "5560" @default.
- W4205697798 abstract "ABSTRACT We post-process galaxies in the IllustrisTNG simulations with skirt radiative transfer calculations to make predictions for the rest-frame near-infrared (NIR) and far-infrared (FIR) properties of galaxies at z ≥ 4. The rest-frame K- and z-band galaxy luminosity functions from TNG are overall consistent with observations, despite ${sim}0.5, mathrm{dex}$ underprediction at z = 4 for MK ≲ −25 and Mz ≲ −24. Predictions for the JWST MIRI observed galaxy luminosity functions and number counts are given. Based on theoretical estimations, we show that the next-generation survey conducted by JWST can detect 500 (30) galaxies in F1000W in a survey area of $500, {rm arcmin}^{2}$ at z = 6 (z = 8). As opposed to the consistency in the UV, optical, and NIR, we find that TNG, combined with our dust modelling choices, significantly underpredicts the abundance of most dust-obscured and thus most luminous FIR galaxies. As a result, the obscured cosmic star formation rate density (SFRD) and the SFRD contributed by optical/NIR dark objects are underpredicted. The discrepancies discovered here could provide new constraints on the sub-grid feedback models, or the dust contents, of simulations. Meanwhile, although the TNG predicted dust temperature and its relations with IR luminosity and redshift are qualitatively consistent with observations, the peak dust temperature of z ≥ 6 galaxies are overestimated by about $20, {rm K}$. This could be related to the limited mass resolution of our simulations to fully resolve the porosity of the interstellar medium (or specifically its dust content) at these redshifts." @default.
- W4205697798 created "2022-01-25" @default.
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- W4205697798 date "2022-01-04" @default.
- W4205697798 modified "2023-10-17" @default.
- W4205697798 title "High-redshift predictions from IllustrisTNG – III. Infrared luminosity functions, obscured star formation, and dust temperature of high-redshift galaxies" @default.
- W4205697798 cites W1494146418 @default.
- W4205697798 cites W1753711873 @default.
- W4205697798 cites W1766563480 @default.
- W4205697798 cites W1851451509 @default.
- W4205697798 cites W1908085087 @default.
- W4205697798 cites W1910580027 @default.
- W4205697798 cites W1911876284 @default.
- W4205697798 cites W1912798299 @default.
- W4205697798 cites W1929623410 @default.
- W4205697798 cites W1964844412 @default.
- W4205697798 cites W1968857920 @default.
- W4205697798 cites W1975549749 @default.
- W4205697798 cites W1979812345 @default.
- W4205697798 cites W1994124960 @default.
- W4205697798 cites W1995047289 @default.
- W4205697798 cites W1999367759 @default.
- W4205697798 cites W2009743038 @default.
- W4205697798 cites W2014678453 @default.
- W4205697798 cites W2015637674 @default.
- W4205697798 cites W2018657673 @default.
- W4205697798 cites W2023717084 @default.
- W4205697798 cites W2024297548 @default.
- W4205697798 cites W2034241894 @default.
- W4205697798 cites W2034608771 @default.
- W4205697798 cites W2035198704 @default.
- W4205697798 cites W2035830593 @default.
- W4205697798 cites W2037187722 @default.
- W4205697798 cites W2037932817 @default.
- W4205697798 cites W2042561599 @default.
- W4205697798 cites W2043279355 @default.
- W4205697798 cites W2049219666 @default.
- W4205697798 cites W2051206400 @default.
- W4205697798 cites W2051885125 @default.
- W4205697798 cites W2056911569 @default.
- W4205697798 cites W2059106820 @default.
- W4205697798 cites W2059302115 @default.
- W4205697798 cites W2073424199 @default.
- W4205697798 cites W2079304679 @default.
- W4205697798 cites W2084178876 @default.
- W4205697798 cites W2108182983 @default.
- W4205697798 cites W2113282530 @default.
- W4205697798 cites W2114951275 @default.
- W4205697798 cites W2115797040 @default.
- W4205697798 cites W2119131940 @default.
- W4205697798 cites W2121931203 @default.
- W4205697798 cites W2121940244 @default.
- W4205697798 cites W2123560671 @default.
- W4205697798 cites W2127377568 @default.
- W4205697798 cites W2139681095 @default.
- W4205697798 cites W2140063909 @default.
- W4205697798 cites W2140887005 @default.
- W4205697798 cites W2141444993 @default.
- W4205697798 cites W2141596435 @default.
- W4205697798 cites W2142220522 @default.
- W4205697798 cites W2146026248 @default.
- W4205697798 cites W2147223987 @default.
- W4205697798 cites W2148804397 @default.
- W4205697798 cites W2150819820 @default.
- W4205697798 cites W2159898631 @default.
- W4205697798 cites W2172214556 @default.
- W4205697798 cites W2183774681 @default.
- W4205697798 cites W2194937049 @default.
- W4205697798 cites W2204815181 @default.
- W4205697798 cites W2296340120 @default.
- W4205697798 cites W2300756355 @default.
- W4205697798 cites W2468373122 @default.
- W4205697798 cites W2468936792 @default.
- W4205697798 cites W2495335077 @default.
- W4205697798 cites W2501238181 @default.
- W4205697798 cites W2522290439 @default.
- W4205697798 cites W2526959632 @default.
- W4205697798 cites W2537447338 @default.
- W4205697798 cites W2577183488 @default.
- W4205697798 cites W2584057118 @default.
- W4205697798 cites W2586579957 @default.
- W4205697798 cites W2589317285 @default.
- W4205697798 cites W2600163159 @default.
- W4205697798 cites W2604350893 @default.
- W4205697798 cites W2612049161 @default.
- W4205697798 cites W2615876086 @default.
- W4205697798 cites W2620847899 @default.
- W4205697798 cites W2702973337 @default.
- W4205697798 cites W2734538553 @default.
- W4205697798 cites W2735189638 @default.
- W4205697798 cites W2735395126 @default.