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The Pan-STARRS1 Medium-Deep Survey: the role of galaxy group environment in the star formation rate versus stellar mass relation and quiescent fraction out to z ~ 0.8

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Phleps,  Stefanie
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Lee,  Chien-Hsiu
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Lin, L., Jian, H.-Y., Foucaud, S., Norberg, P., Bower, R. G., Cole, S., Arnalte-Mur, P., Chen, C.-W., Coupon, J., Hsieh, B.-C., Heinis, S., Phleps, S., Chen, W.-P., Lee, C.-H., Burgett, W., Chambers, K. C., Denneau, L., Draper, P., Flewelling, H., Hodapp, K. W., Huber, M. E., Kaiser, N., Kudritzki, R.-P., Magnier, E. A., Metcalfe, N., Price, P. A., Tonry, J. L., Wainscoat, R. J., & Waters, C. (2014). The Pan-STARRS1 Medium-Deep Survey: the role of galaxy group environment in the star formation rate versus stellar mass relation and quiescent fraction out to z ~ 0.8. The Astrophysical Journal, 782(1):, pp. 1-16. doi:10.1088/0004-637X/782/1/33.


引用: https://hdl.handle.net/11858/00-001M-0000-0019-1A4A-D
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