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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 3.

Compilation of samples from the literature used in this analysis with their redshifts and elevation above the MS as parameterized by δMS = sSFR/﹩\langle {\mathrm{sSFR}}_{\mathrm{MS}}\rangle ﹩ and described in Section 4. Our ALMA sample of 12 starbursts is shown by the larger red circles. Further details are provided in the text, including a more extensive set of references to these data sets.

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