SDSS IV MaNGA - the spatially resolved transition from star formation to quiescence
SDSS IV MaNGA - the spatially resolved transition from star formation to quiescence
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DOI:
10.1093/mnras/stw3211
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发表时间:
2016-09
影响因子:
4.8
通讯作者:
F. Belfiore;R. Maiolino;C. Maraston;E. Emsellem;M. Bershady;K. Masters;D. Bizyaev;M. Boquien;J. Brownstein;K. Bundy;A. Diamond-Stanic;N. Drory;T. Heckman;D. Law;O. Malanushenko;A. Oravetz;K. Pan;A. Roman-Lopes;D. Thomas;A. Weijmans;K. Westfall;R. Yan
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作者:
F. Belfiore;R. Maiolino;C. Maraston;E. Emsellem;M. Bershady;K. Masters;D. Bizyaev;M. Boquien;J. Brownstein;K. Bundy;A. Diamond-Stanic;N. Drory;T. Heckman;D. Law;O. Malanushenko;A. Oravetz;K. Pan;A. Roman-Lopes;D. Thomas;A. Weijmans;K. Westfall;R. Yan
FB, RM and KM acknowledge funding from the United Kingdom Science and Technology Facilities Council (STFC). RM acknowledges support from the European Research Council (ERC) Advanced Grant 695671 ‘QUENCH’. AR-L acknowledges partial support from the DIULS regular project PR15143. MB was supported by NSF/AST-1517006. KB was supported by World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan and by JSPS KAKENHI Grant Number 15K17603. AW acknowledges support from a Leverhulme Early Career Fellowship. AD acknowledges support from The Grainger Foundation.