Diffuse Lyα haloes around Lyα emitters at z=3: do dark matter distributions determine the Lyα spatial extents?

Author:

Matsuda Y.,Yamada T.1,Hayashino T.2,Yamauchi R.2,Nakamura Y.,Morimoto N.1,Ouchi M.3,Ono Y.4,Umemura M.5,Mori M.5

Affiliation:

1. Astronomical Institute, Graduate School of Science; Tohoku University; Aramaki, Aoba-ku; Sendai; 980-8578; Japan

2. Research Center for Neutrino Science, Graduate School of Science; Tohoku University; Sendai; 980-8578; Japan

3. Institute for Cosmic Ray Research; University of Tokyo; Kashiwa; 277-8582; Japan

4. Department of Astronomy, Graduate School of Science; University of Tokyo; Tokyo; 113-0033; Japan

5. Center for Computational Sciences; University of Tsukuba; Tsukuba; 305-8577; Japan

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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