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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 7.

Distributions of basic properties for all our XMPGs (blue) and [O III]λ4363-detected galaxies (red), including redshift (a), r-band magnitude in mag (b), gas-phase extinction E(B − V) in mag (c), electron density N e (d) in the unit of per cubic centimeter, electron temperature T e in K (e), logarithmic equivalent width of [O III]λ5007 in angstrom (f), logarithmic SFR in M ⊙ yr−1 (g), logarithmic stellar mass in M ⊙ (h), and logarithmic sSFR per year (i).

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