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The FMOS-COSMOS Survey of Star-forming Galaxies at z ∼ 1.6. VI. Redshift and Emission-line Catalog and Basic Properties of Star-forming Galaxies

  • Authors: Daichi Kashino, John D. Silverman, David Sanders, Jeyhan Kartaltepe, Emanuele Daddi, Alvio Renzini, Giulia Rodighiero, Annagrazia Puglisi, Francesco Valentino, Stéphanie Juneau, Nobuo Arimoto, Tohru Nagao, Olivier Ilbert, Olivier Le Fèvre, and Anton. M. Koekemoer

2019 The Astrophysical Journal Supplement Series 241 10.

  • Provider: AAS Journals

Caption: Figure 32.

Best-fit M* vs. SFR relations for the FMOS objects, in comparison to literature measurements. Pale colored circles indicate FMOS objects (same as in Figure 31). Thick solid curves indicate the best-fit relations to the FMOS data: power-law fits to objects with ﹩\mathrm{log}{M}_{* }/{M}_{\odot }\geqslant 9.6﹩ (gray) and ﹩9.6\,\leqslant \mathrm{log}{M}_{* }/{M}_{\odot }\leqslant 10.6﹩ (green), asymptotic function fit (red), and broken power-law fit (blue). Colored dashed lines indicate literature measurements: fit to a subset of the FMOS sample (Kashino et al. 2013; green), broken power-law fit at ﹩1.5\leqslant z\leqslant 2.0﹩ from Whitaker et al. (2014; blue), and asymptotic function fit at median ﹩\left\langle z\right\rangle =1.19﹩ from Lee et al. (2015; red). Three dashed gray lines indicate an empirically parameterized relation at z = 0.1, 0.8, and 1.6 (top to bottom) derived by Speagle et al. (2014).

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