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UV and Lyα Halos of Lyα Emitters across Environments at z = 2.84

  • Authors: Satoshi Kikuta, Yuichi Matsuda, Shigeki Inoue, Charles C. Steidel, Renyue Cen, Zheng Zheng, Hidenobu Yajima, Rieko Momose, Masatoshi Imanishi, Yutaka Komiyama

Satoshi Kikuta et al 2023 The Astrophysical Journal 947 .

  • Provider: AAS Journals

Caption: Figure 1.

Sky distribution of our LAEs (colored dots). The HLQSO is located at the origin (0,0). North is up, and east to the left. The colors indicate their rest-frame Lyα equivalent width, and the sizes indicate their UV absolute magnitude (the larger, the brighter). Gray contours indicate their overdensity δ, with each level showing a different group defined in Table 1. Concentric black circles indicate radii with which the distance subsamples are defined.

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