Figure 2 from The Molecular Gas Content and Fuel Efficiency of Starbursts at z ∼ 1.6 with ALMA

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The Molecular Gas Content and Fuel Efficiency of Starbursts at z ∼ 1.6 with ALMA

Authors: J. D. Silverman, W. Rujopakarn, E. Daddi, A. Renzini, G. Rodighiero, D. Liu, A. Puglisi, M. Sargent, C. Mancini, J. Kartaltepe, D. Kashino, A. Koekemoer, N. Arimoto, M. Béthermin, S. Jin, G. Magdis, T. Nagao, M. Onodera, D. Sanders, and F. Valentino

2018 The Astrophysical Journal 867 92.

Provider: AAS Journals

Caption: Figure 2.

SEDs of our Cycle 3 sample from IR to radio wavelengths (photometric data are shown in blue), with the best-fit model shown by the black curve. The model of the dust emission is given for both a warm (red) and a cool (purple) component that contributes to the mid- to far-infrared emission. The unobscured stellar emission is shown by the cyan curve. An AGN contribution (yellow) is negligible for all cases.

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