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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 38.

Distribution of the [N II] λ6584/Hα ratios normalized to the best-fit relation at a given M*. Objects in the FMOS Sample-H, having both Hα and [N II] detections, are shown by filled histograms in four ranges of stellar mass: log M*/M = [9.2:11.5] (upper left), [9.2:10.0] (upper right), [10.0:10.6] (lower left), and [10.6:11.5] (lower right). Black open histograms indicate the distribution of upper limits. The numbers of all Hα-detected galaxies (regardless of [N II] detection; N(Hα)) and those with both Hα and [N II] detections (N(Hα + [N II])) within the mass ranges are given in each panel. The red curve indicates a zero-mean normal function with a broadened standard deviation of ﹩\sigma =\sqrt{{\sigma }_{\mathrm{int}}^{2}+{\left\langle \delta \right\rangle }^{2}}﹩. The values of σ, σint, and the median errors ﹩\left\langle \delta \right\rangle ﹩ are given in each panel.

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