The Intrinsic Characteristics of Galaxies on the SFR–M ∗ Plane at 1.2 < z < 4: I. The Correlation between Stellar Age, Central Density, and Position Relative to the Main Sequence

The Intrinsic Characteristics of Galaxies on the SFR–M ∗ Plane at 1.2 < z < 4: I. The Correlation between Stellar Age, Central Density, and Position Relative to the Main Sequence

We use the deep CANDELS observations in the GOODS North and South fields to revisit the correlations between stellar mass (M-*), star formation rate (SFR) and morphology, and to introduce a fourth dimension, the mass-weighted stellar age, in galaxies at 1.2 < z < 4. We do this by making new me...

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Bibliographic Details
Main Authors: Lee, Bomee, Giavalisco, Mauro, Whitaker, Katherine, Williams, Christina C., Ferguson, Henry C., Acquaviva, Viviana, Koekemoer, Anton M., Straughn, Amber N., Guo, Yicheng, Kartaltepe, Jeyhan S., Lotz, Jennifer, Pacifici, Camilla, Croton, Darren J., Somerville, Rachel S., Lu, Yu
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2018
Subjects:
galaxies: evolution
galaxies: formation
Galaxy: structure
techniques: photometric
Online Access:http://hdl.handle.net/10150/627039
http://arizona.openrepository.com/arizona/handle/10150/627039

Internet

http://hdl.handle.net/10150/627039
http://arizona.openrepository.com/arizona/handle/10150/627039

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