Abstract
MAHALO-Subaru (MApping HAlpha and Lines of Oxygen with Subaru) is our on-going large programme which aims to investigate how the star forming activities in galaxies are propagated as a function of time, mass, and environment. We are targeting 10 clusters and proto-clusters at 0.4 2, which suggests that the mode of star formation and/or the activation of AGN are dependent on environment, and thus holding the key to the environmental effects at the early stage of cluster galaxies formation and evolution. © 2013 International Astronomical Union.
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Kodama, T., Hayashi, M., Koyama, Y., Tadaki, K. I., Tanaka, I., & Shimakawa, R. (2012). Mahalo-subaru: Mapping star formation at the peak epoch of massive galaxy formation. In Proceedings of the International Astronomical Union (Vol. 8, pp. 74–77). https://doi.org/10.1017/S1743921313004353
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