Predicted UV-to-Radio SEDs of little red dots: AGN and SF
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Predicted Dust SEDs for JWST's Little Red Dots17-Sep-2024 Here are the average UV through radio spectral energy distributions predicted for the LRD population from Figure 2 of Casey et al. (2024b, https://arxiv.org/abs/2407.05094, ApJL in press). There are two SEDs: one predicting the emission is due to AGN and one that it is due to star-formation. Wavelength is given as log10 of rest-frame wavelength in microns. Flux density is log10 Fnu in mJy. Email cmcasey.astro@gmail.com with questions.
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2024-09-17
