Image Details
Caption: Figure 7.
The three JWST data points (one NIRCam and two MIRI) for the source S1 are compared with illustrative SEDs of a number of extragalactic objects (from a suite of Spitzer SWIRE templates; M. Polletta et al. 2007) and with the spectrum of cloudless T eff = 200 K, log (g) = 3 Sonora Bobcat model (M. S. Marley et al. 2021).
© 2024. The Author(s). Published by the American Astronomical Society.