The Physical Properties of Star-forming Galaxies with Strong [O iii] Lines at z = 3.25

@article{Wen2022ThePP,
  title={The Physical Properties of Star-forming Galaxies with Strong [O iii] Lines at z = 3.25},
  author={Run Wen and Fangxia An and Xianzhong Zheng and Dongdong Shi and Jianbo Qin and Valentino Gonzalez and Fuyan Bian and Haiguang Xu and Zhizheng Pan and Qinghua Tan and Wenhao Liu and Min Fang and Jian Ren and Yu Heng Zhang and Man Qiao and Shuang Liu},
  journal={The Astrophysical Journal},
  year={2022},
  volume={933}
}
We present an analysis of physical properties of 34 [O iii] emission-line galaxies (ELGs) at z = 3.254 ± 0.029 in the Extended Chandra Deep Field South (ECDFS). These ELGs are selected from deep narrow H2S(1) and broad K s imaging of 383 arcmin2 obtained with CFHT/WIRCam. We construct spectral energy distributions (SEDs) from U to K s to derive the physical properties of ELGs. These [O iii] ELGs are identified as starburst galaxies with strong [O iii] lines of L OIII ∼ 1042.6–1044.2 erg s−1 and… 

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