Matches in SemOpenAlex for { <https://semopenalex.org/work/W3008659311> ?p ?o ?g. }
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- W3008659311 abstract "We present predictions for high redshift ($z=2-10$) galaxy populations based on the IllustrisTNG simulation suite and a full Monte Carlo dust radiative transfer post-processing. Specifically, we discuss the ${rm H}_{alpha}$ and ${rm H}_{beta}$ + $[rm O ,III]$ luminosity functions up to $z=8$. The predicted ${rm H}_{beta}$ + $[rm O ,III]$ luminosity functions are consistent with present observations at $zlesssim 3$ with $lesssim 0.1,{rm dex}$ differences in luminosities. However, the predicted ${rm H}_{alpha}$ luminosity function is $sim 0.3,{rm dex}$ dimmer than the observed one at $zsimeq 2$. Furthermore, we explore continuum spectral indices, the Balmer break at $4000$AA (D4000) and the UV continuum slope $beta$. The median D4000 versus sSFR relation predicted at $z=2$ is in agreement with the local calibration despite a different distribution pattern of galaxies in this plane. In addition, we reproduce the observed $A_{rm UV}$ versus $beta$ relation and explore its dependence on galaxy stellar mass, providing an explanation for the observed complexity of this relation. We also find a deficiency in heavily attenuated, UV red galaxies in the simulations. Finally, we provide predictions for the dust attenuation curves of galaxies at $z=2-6$ and investigate their dependence on galaxy colors and stellar masses. The attenuation curves are steeper in galaxies at higher redshifts, with bluer colors, or with lower stellar masses. We attribute these predicted trends to dust geometry. Overall, our results are consistent with present observations of high redshift galaxies. Future JWST observations will further test these predictions." @default.
- W3008659311 created "2020-03-06" @default.
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- W3008659311 date "2020-05-22" @default.
- W3008659311 modified "2023-10-12" @default.
- W3008659311 title "High-redshift <i>JWST</i> predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves" @default.
- W3008659311 cites W1484039435 @default.
- W3008659311 cites W1494146418 @default.
- W3008659311 cites W1508863994 @default.
- W3008659311 cites W1529219299 @default.
- W3008659311 cites W1753711873 @default.
- W3008659311 cites W1791877437 @default.
- W3008659311 cites W1842880767 @default.
- W3008659311 cites W1850248739 @default.
- W3008659311 cites W1908085087 @default.
- W3008659311 cites W1911876284 @default.
- W3008659311 cites W1912798299 @default.
- W3008659311 cites W1962697969 @default.
- W3008659311 cites W1964844412 @default.
- W3008659311 cites W1972232491 @default.
- W3008659311 cites W1972726718 @default.
- W3008659311 cites W1974174849 @default.
- W3008659311 cites W1975549749 @default.
- W3008659311 cites W1981829125 @default.
- W3008659311 cites W1986549462 @default.
- W3008659311 cites W1994771289 @default.
- W3008659311 cites W1995836635 @default.
- W3008659311 cites W1996926090 @default.
- W3008659311 cites W1997151814 @default.
- W3008659311 cites W1999367759 @default.
- W3008659311 cites W2000840256 @default.
- W3008659311 cites W2008047915 @default.
- W3008659311 cites W2008991538 @default.
- W3008659311 cites W2013951064 @default.
- W3008659311 cites W2017689889 @default.
- W3008659311 cites W2019615555 @default.
- W3008659311 cites W2034241894 @default.
- W3008659311 cites W2037187722 @default.
- W3008659311 cites W2037526471 @default.
- W3008659311 cites W2037932817 @default.
- W3008659311 cites W2041084195 @default.
- W3008659311 cites W2042561599 @default.
- W3008659311 cites W2042994140 @default.
- W3008659311 cites W2048274049 @default.
- W3008659311 cites W2048678471 @default.
- W3008659311 cites W2052923345 @default.
- W3008659311 cites W2053265856 @default.
- W3008659311 cites W2054041840 @default.
- W3008659311 cites W2058387099 @default.
- W3008659311 cites W2059302115 @default.
- W3008659311 cites W2062398112 @default.
- W3008659311 cites W2063601622 @default.
- W3008659311 cites W2063814094 @default.
- W3008659311 cites W2070696493 @default.
- W3008659311 cites W2071407353 @default.
- W3008659311 cites W2073424199 @default.
- W3008659311 cites W2074259895 @default.
- W3008659311 cites W2077054687 @default.
- W3008659311 cites W2079304679 @default.
- W3008659311 cites W2080927107 @default.
- W3008659311 cites W2084178876 @default.
- W3008659311 cites W2086328762 @default.
- W3008659311 cites W2086913701 @default.
- W3008659311 cites W2087459521 @default.
- W3008659311 cites W2091010926 @default.
- W3008659311 cites W2093998251 @default.
- W3008659311 cites W2094181926 @default.
- W3008659311 cites W2095044009 @default.
- W3008659311 cites W2101405699 @default.
- W3008659311 cites W2109062722 @default.
- W3008659311 cites W2114951275 @default.
- W3008659311 cites W2115797040 @default.
- W3008659311 cites W2121173473 @default.
- W3008659311 cites W2121940244 @default.
- W3008659311 cites W2124924585 @default.
- W3008659311 cites W2134403072 @default.
- W3008659311 cites W2135221285 @default.
- W3008659311 cites W2140887005 @default.
- W3008659311 cites W2144632906 @default.
- W3008659311 cites W2146026248 @default.
- W3008659311 cites W2150819820 @default.
- W3008659311 cites W2151062050 @default.
- W3008659311 cites W2155805383 @default.
- W3008659311 cites W2158622701 @default.
- W3008659311 cites W2159898631 @default.
- W3008659311 cites W2165375085 @default.
- W3008659311 cites W2166365370 @default.
- W3008659311 cites W2167635287 @default.
- W3008659311 cites W2170912300 @default.
- W3008659311 cites W2172214556 @default.