Mass assembly and morphological transformations since z∼ 3 from CANDELS

Mass assembly and morphological transformations since z∼ 3 from CANDELS

We quantify the evolution of the stellar mass functions (SMFs) of star-forming and quiescent galaxies as a function of morphology from z ∼ 3 to the present. Our sample consists of ∼50 000 galaxies in the CANDELS fields (∼880 arcmin2), which we divide into four main morphological types, i.e. pure bul...

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Bibliographic Details
Main Authors: Huertas-Company, M., Bernardi, M., Pérez-González, P.G., Ashby, M.L.N., Barro, G., Conselice, Christopher J., Daddi, E., Dekel, A., Dimauro, P., Faber, S.M., Grogin, N.A., Kartaltepe, J.S., Kocevski, D.D., Koekemoer, A.M., Koo, D.C., Mei, S., Shankar, F.
Format: Article
Published: Oxford University Press 2016
Subjects:
galaxies: abundances
galaxies: evolution
galaxies: high-redshift
galaxies: structure.
Online Access:https://eprints.nottingham.ac.uk/39570/

Internet

https://eprints.nottingham.ac.uk/39570/

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