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[O iii] emission line as a tracer of star-forming galaxies at high redshifts: comparison between Hα and [O iii] emitters at z=2.23 in HiZELS by Suzuki, T. L. (author);Kodama, T. (author);Sobral, D. (author);Khostovan, A. A. (author);Hayashi, M. (author);Shimakawa, R. (author);Koyama, Y. (author);Tadaki, K. I. (author);Tanaka, I. (author);Minowa, Y. (author);Yamamoto, M. (author);Smail, I. (author);Best, P. N. (author) is a Physics and Astronomy article available to read on EtoBox.

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Author
Suzuki, T. L. (author);Kodama, T. (author);Sobral, D. (author);Khostovan, A. A. (author);Hayashi, M. (author);Shimakawa, R. (author);Koyama, Y. (author);Tadaki, K. I. (author);Tanaka, I. (author);Minowa, Y. (author);Yamamoto, M. (author);Smail, I. (author);Best, P. N. (author)
Publisher
Oxford University Press
Published
2016
Field
Physics and Astronomy (Physical Sciences)

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