Shapley supercluster survey: galaxy evolution from filaments to cluster cores
Shapley supercluster survey: galaxy evolution from filaments to cluster cores
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DOI：
10.1093/mnras/stu2085
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发表时间：
2014-07
影响因子：
4.8
通讯作者：
P. Merluzzi;G. Busarello;C. Haines;A. Mercurio;Nobuhiro Okabe;K. Pimbblet;K. Pimbblet;M. Dopita
中科院分区：
文献类型：
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作者：
P. Merluzzi;G. Busarello;C. Haines;A. Mercurio;Nobuhiro Okabe;K. Pimbblet;K. Pimbblet;M. Dopita
导致这些结果的研究已经收到了来自欧洲共同体第七框架计划（FP 7/2007-13）的资助，资助协议编号为312430（OPTICON; PI：P. Merluzzi）和PRIN-INAF 2011“VLT巡天望远镜（VST）的星系演化”（PI A。格拉多）。CPH由CONICYT Anillo项目ACT-1122资助。N.Okabe得到了日本文部科学省（26800097）和日本文部科学省世界一流国际研究中心倡议（WPI倡议）的资助。
The research leading to these results has received funding from the European Community’s Seventh Framework Programme (FP7/2007–13) under grant agreement number 312430 (OPTICON; PI: P. Merluzzi) and PRIN-INAF 2011 ‘Galaxy evolution with the VLT Surveys Telescope (VST)’ (PI A. Grado). CPH was funded by CONICYT Anillo project ACT-1122. N.Okabe is supported by a Grant-in-Aid from the Ministry of Education, Culture, Sports, Science and Technology of Japan (26800097) and by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan.