Image Details
Caption: Figure 8.
Fits of the NIRCam, MIRI, and ALMA data for source #1 to a series of SWIRE templates for extragalactic source types (L. Silva et al. 1998; M. Polletta et al. 2007). The NIRcam data for the two resolved components are combined in this fit. AGN and/or starburst sources provide qualitative fits to the spectral energy distribution.
© 2026. The Author(s). Published by the American Astronomical Society.