Figure 3 from POWDERDAY: Dust Radiative Transfer for Galaxy Simulations

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POWDERDAY: Dust Radiative Transfer for Galaxy Simulations

Authors: Desika Narayanan, Matthew J. Turk, Thomas Robitaille, Ashley J. Kelly, B. Connor McClellan, Ray S Sharma, Prerak Garg, Matthew Abruzzo, Ena Choi, Charlie Conroy, Benjamin D. Johnson, Benjamin Kimock, Qi Li, Christopher C. Lovell, Sidney Lower, George C. Privon, Jonathan Roberts, Snigdaa Sethuram, Gregory F. Snyder, Robert Thompson, and John H. Wise

2021 The Astrophysical Journal Supplement Series 252 12.

Provider: AAS Journals

Caption: Figure 3.

Example of possible input SEDs for accreting black holes. The blue line shows the Hopkins et al. (2007) template SED, while the orange line shows the Nenkova et al. (2008b) model. The green line shows the output observed SED (including the contribution from stars and dust).

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