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COMAP Early Science. VI. A First Look at the COMAP Galactic Plane Survey

Authors: Thomas J. Rennie, Stuart E. Harper, Clive Dickinson, Liju Philip, Kieran A. Cleary, Richard J. Bond, Jowita Borowska, Patrick C. Breysse, Morgan Catha, Roke Cepeda-Arroita, Dongwoo T. Chung, Sarah E. Church, Delaney A. Dunne, Hans Kristian Eriksen, Marie Kristine Foss, Todd Gaier, Joshua Ott Gundersen, Andrew I. Harris, Brandon Hensley, Richard Hobbs, Håvard T. Ihle, James W. Lamb, Charles R. Lawrence, Jonas G. S. Lunde, Roberta Paladini, Timothy J. Pearson, Maren Rasmussen, Anthony C. S. Readhead, Nils-Ole Stutzer, Duncan J. Watts, Ingunn Kathrine Wehus, David P. Woody

Thomas J. Rennie et al 2022 The Astrophysical Journal 933 .

Provider: AAS Journals

Caption: Figure 5.

SEDs of six H II regions that show a significant AME detection. Filled circles are used in the fit while open circles are not. The free–free, spinning dust, and thermal dust components are shown as dashed, dashed–dotted, 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.

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