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A Large Sample of Extremely Metal-poor Galaxies at z < 1 Identified from the DESI Early Data

  • Authors: Hu Zou, Jipeng Sui, Amélie Saintonge, Dirk Scholte, John Moustakas, Malgorzata Siudek, Arjun Dey, Stephanie Juneau, Weijian Guo, Rebecca Canning, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, K. Dawson, A. de la Macorra, P. Doel, J. E. Forero-Romero, S. Gontcho A Gontcho, K. Honscheid, M. Landriau, L. Le Guillou, M. Manera, A. Meisner, R. Miquel, Jundan Nie, C. Poppett, M. Rezaie, G. Rossi, E. Sanchez, M. Schubnell, H. Seo, G. Tarlé, Zhimin Zhou, Siwei Zou

Hu Zou et al 2024 The Astrophysical Journal 961 .

  • Provider: AAS Journals

Caption: Figure 3.

BPT diagnostic diagrams to discriminate star-forming galaxies (blue dots) from AGNs (red crosses). These galaxies shown are [O III]λ4363 detected. (a) The BPT diagram of [O III]λ5007/Hβ vs. [N II]λ6583/Hα. The dashed line shows the empirical division between starbursts and AGNs obtained by Kauffmann et al. (2003). (b) The BPT diagram of [O III]/Hβ vs. [S II]/Hα. The dashed line shows the theoretical division between starbursts and AGNs obtained by Kewley et al. (2001). The solid lines in these two panels display the demarcation curves with an additional uncertainty of 0.1 dex. (c) The galaxy distribution on the plot of [O III]λ5007/Hβ vs. [O II]/Hβ. The dashed line presents the separation limit proposed by Lamareille (2010). The solid line displays the separation limit with the addition of an extra 0.15 dex uncertainty, which is used as our new proposed demarcation between starbursts and AGNs.

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