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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 42.

Distribution of Hα and [O III] λ5007 fluxes (corrected for aperture loss but not for dust extinction) in different bins of M*:log M*/M = [9.0:9.9] (upper left), [9.9:10.3] (upper right), [10.3:10.7] (lower left), and ≥10.7 (lower right). Open histograms indicate the FHα distribution for the Hα emitters. Red filled and blue hatched histograms indicate distributions of Hα and [O III] λ5007 fluxes, respectively, for the Hα+[O III]-emitter sample. In each panel, we give the number of Hα and Hα+[O III] emitters (e.g., in the upper left panel, the numbers of Hα and Hα+[O III] emitters within the bin are 185 and 102 (55%), respectively), as well as the median values of the observed Hα and [O III] fluxes in log scale in units of ﹩{10}^{-17}\,\mathrm{erg}\,{{\rm{s}}}^{-1}\,{\mathrm{cm}}^{-2}﹩.

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