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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 10.

Stacked Lyα (left, orange) and continuum (right, blue) images of different subsamples in the asinh color stretch. From top to bottom, we show stacked images of UV magnitude, L Lyα , EW0,Lyα , distance from the HLQSO, and environment subsamples. From left to right, median [UV magnitude, L Lyα , EW0,Lyα , distance from the HLQSO, δ] of each subsample respectively become [fainter, fainter, larger, larger, smaller]. The size of each image is ∼200 × 200 pkpc. Contours correspond to ﹩3\times {10}^{-18},1\times {10}^{-18},1\times {10}^{-19}\,\mathrm{erg}\,{{\rm{s}}}^{-1}\,{\mathrm{cm}}^{-2}\,{\mathrm{arcsec}}^{-2}﹩ in the Lyα images and ﹩3\times {10}^{-31},1\times {10}^{-31},3\times {10}^{-32}\,\mathrm{erg}\,{{\rm{s}}}^{-1}\,{\mathrm{cm}}^{-2}\,{\mathrm{Hz}}^{-1}\,{\mathrm{arcsec}}^{-2}﹩ in continuum images.

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