Stacking analysis of Euclid Q1 galaxies with Herschel/SCUBA-2 data yields average dust temperatures following T2 + (T1-T2)exp(-t/τ) converging to ~23 K at low redshift, decreasing dust-to-stellar mass ratios, and >60% contribution to the CIB at 250-500 μm.
M., Narayanan , D., & Cooray , A
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RTGen applies post-processing Monte Carlo radiative transfer to six hydrodynamic galaxy simulations to compute dust temperatures, SEDs, continuum images, and molecular line emission while testing the effects of dust modeling choices.
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Euclid Quick Data Release (Q1). The average far-infrared properties of Euclid-selected star-forming galaxies
Stacking analysis of Euclid Q1 galaxies with Herschel/SCUBA-2 data yields average dust temperatures following T2 + (T1-T2)exp(-t/τ) converging to ~23 K at low redshift, decreasing dust-to-stellar mass ratios, and >60% contribution to the CIB at 250-500 μm.
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Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
RTGen applies post-processing Monte Carlo radiative transfer to six hydrodynamic galaxy simulations to compute dust temperatures, SEDs, continuum images, and molecular line emission while testing the effects of dust modeling choices.