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The KMOS GTO cluster program: absorption line spectroscopy of cluster galaxies at z∼1.5

MPS-Authors
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Bender,  R.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Beifiori,  A.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Chan,  J.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Galametz,  A.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Mendel,  J. T.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Saglia,  R. P.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Wilman,  D.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Houghton, R. C. W., Davies, R. L., Bender, R., Beifiori, A., Chan, J., Cappellari, M., et al. (2016). The KMOS GTO cluster program: absorption line spectroscopy of cluster galaxies at z∼1.5. In I. Skillen, M. Balcells, & S. C. Trager (Eds.), Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields (pp. 281-285).


Cite as: https://hdl.handle.net/11858/00-001M-0000-002C-A11B-A
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