The physical properties of massive green valley galaxies as a function of environments at $0.5 postprint

Author: Wenjun Chang Guanwen Fang Yizhou Gu Zesen Lin Shiying Lu Xu Kong
Submit Time:2023-02-19 20:58:59

Abstract: To investigate the effects of environment in the quenching phase, we study the empirical relations for green valley (GV) galaxies between overdensity and other physical properties (i.e., effective radius $r_{\rm e}$, S\'{e}rsic indices $n$, and specific star formation rate sSFR). Based on five 3D-{\it HST}/CANDELS fields, we construct a large sample of 2126 massive ($M_{\star} > 10^{10} M_{\sun}$) GV galaxies at $0.5

Subject: Astronomy >> Astrophysical processes
Cite as: ChinaXiv:202303.05150 (or this version ChinaXiv:202303.05150V1)
DOI:10.12074/202303.05150V1
CSTR:32003.36.ChinaXiv.202303.05150.V1
TXID： 3454456e-ae58-40da-a8bc-3a60e1789f50
Recommended references： Wenjun Chang,Guanwen Fang,Yizhou Gu,Zesen Lin,Shiying Lu,Xu Kong.The physical properties of massive green valley galaxies as a function of environments at $0.5 (Click&Copy)

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2023-02-19 20:58:59

ChinaXiv:202303.05150V1

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The physical properties of massive green valley galaxies as a function of environments at $0.5 postprint

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