Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust by Kannan, Rahul, Marinacci, Federico, Vogelsberger, Mark, Sales, Laura V, Torrey, Paul, Springel, Volker, Hernquist, Lars

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Hydrogen reionization in the Illustris universe by Bauer, Andreas, Springel, Volker, Vogelsberger, Mark, Genel, Shy, Torrey, Paul, Sijacki, Debora, Nelson, Dylan, Hernquist, Lars

“…Furthermore, we show that moment-based approaches for radiative transfer with the M1 closure give broadly consistent results with our angular-resolved radiative transfer scheme. …”
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The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations by Rodriguez-Gomez, Vicente, Snyder, Gregory F, Lotz, Jennifer M, Nelson, Dylan, Pillepich, Annalisa, Springel, Volker, Genel, Shy, Weinberger, Rainer, Tacchella, Sandro, Pakmor, Rüdiger, Torrey, Paul, Marinacci, Federico, Vogelsberger, Mark, Hernquist, Lars, Thilker, David A

“…Most of our synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering, and performing the radiative transfer directly on the Voronoi mesh used by the simulations themselves. …”
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High-redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves by Shen, Xuejian, Vogelsberger, Mark, Nelson, Dylan, Pillepich, Annalisa, Tacchella, Sandro, Marinacci, Federico, Torrey, Paul, Hernquist, Lars, Springel, Volker

“…<jats:title>ABSTRACT</jats:title> <jats:p>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 H α and H β + $[\rm O \,{\small III}]$ luminosity functions up to z = 8. …”
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High-redshift JWST predictions from IllustrisTNG: dust modelling and galaxy luminosity functions by Vogelsberger, Mark, Nelson, Dylan, Pillepich, Annalisa, Shen, Xuejian, Marinacci, Federico, Springel, Volker, Pakmor, Rüdiger, Tacchella, Sandro, Weinberger, Rainer, Torrey, Paul, Hernquist, Lars

“…Our most detailed dust model is based on continuum Monte Carlo radiative transfer calculations employing observationally calibrated dust properties. …”
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High-redshift JWST predictions from IllustrisTNG: dust modelling and galaxy luminosity functions by Vogelsberger, Mark, Nelson, Dylan, Pillepich, Annalisa, Shen, Xuejian, Marinacci, Federico, Springel, Volker, Pakmor, Rüdiger, Tacchella, Sandro, Weinberger, Rainer, Torrey, Paul A., Hernquist, Lars

“…Our most detailed dust model is based on continuum Monte Carlo radiative transfer calculations employing observationally calibrated dust properties. …”
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High-redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves by Shen, Xuejian, Vogelsberger, Mark, Nelson, Dylan, Pillepich, Annalisa, Tacchella, Sandro, Marinacci, Federico, Torrey, Paul A., Hernquist, Lars, Springel, Volker

“…<jats:title>ABSTRACT</jats:title> <jats:p>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 H α and H β + $[\rm O \,{\small III}]$ luminosity functions up to z = 8. …”
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High-redshift predictions from IllustrisTNG – III. Infrared luminosity functions, obscured star formation, and dust temperature of high-redshift galaxies by Shen, Xuejian, Vogelsberger, Mark, Nelson, Dylan, Tacchella, Sandro, Hernquist, Lars, Springel, Volker, Marinacci, Federico, Torrey, Paul

“…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. …”
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Submillimetre galaxies in cosmological hydrodynamical simulations – an opportunity for constraining feedback models by Hayward, Christopher C, Sparre, Martin, Chapman, Scott C, Hernquist, Lars, Nelson, Dylan, Pakmor, Rüdiger, Pillepich, Annalisa, Springel, Volker, Torrey, Paul, Vogelsberger, Mark, Weinberger, Rainer

“…We use a scaling relation derived from previous simulations plus radiative transfer calculations to predict the submm flux densities of simulated SMGs drawn from cosmological simulations from the Illustris and IllustrisTNG projects based on the simulated galaxies’ star formation rates (SFRs) and dust masses, and compare the predicted number counts with observations. …”
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