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Strong [O III] λ5007 Compact Galaxies Identified from SDSS DR16 and Their Scaling Relations

  • Authors: Weiyu Ding, Hu Zou, Xu Kong, Yulong Gao, Fujia Li, Hongxin Zhang, Jiali Wang, Jie Song, Jipeng Sui, Jundan Nie, Suijian Xue, Weijian Guo, Yao Yao, Zhimin Zhou

Weiyu Ding et al 2023 The Astronomical Journal 166 .

  • Provider: AAS Journals

Caption: Figure 6.

Relation between stellar mass and SFR for our strong [O III]λ5007 compact galaxies (filled circles) color-coded by redshift. The error bars in orange show the measurement uncertainties. Blueberry galaxies (light blue pentagons) from Yang et al. (2017b), green-pea galaxies from Cardamone et al. (2009; green triangles), Brunker et al. (2020; purple stars), Yang et al. (2017a; gray diamonds), and Tacchella et al. (2022; black cross) are also overplotted. The star-forming main sequence for normal galaxies at redshift of z = 0.11 from Speagle et al. (2014) is plotted in dashed line for comparison and the red shade indicates the uncertainty of this SFMS. The solid line represents the best robust linear fitting to our galaxy sample. The dotted lines present the constant sSFRs of 10−7, 10−8, 10−9, and 10−10 yr−1.

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