Image Details
Caption: Figure 4.
SEDs of three H II regions without an AME detection. Filled circles are used in the fit while open circles are not. The free–free and thermal dust components are shown as dashed and dotted lines, respectively. The total emission model is shown as a thick red line. The inset shown on the upper left of all plots shows the COMAP in-band 26–34 GHz spectrum.
© 2022. The Author(s). Published by the American Astronomical Society.