Rachel Asquith
Cosmic CARNage II: the evolution of the galaxy stellar mass functionin observations and galaxy formation models
Asquith, Rachel; Pearce, Frazer R.; Almaini, Omar; Knebe, Alexander; Gonzalez-Perez, Violeta; Benson, Andrew; Blaizot, Jeremy; Carretero, Jorge; Castander, Francisco J.; Cattaneo, Andrea; Cora, Sofía A; Croton, Darren J.; Devriendt, Julien E.; Fontanot, Fabio; Gargiulo, Ignacio D.; Hartley, Will; Henriques, Bruno; Lee, Jaehyun; Mamon, Gary A.; Onions, Julian; Padilla, Nelson D.; Power, Chris; Srisawat, Chaichalit; Stevens, Adam R.H.; Thomas, Peter A.; Vega-Martínez, Cristian A.; Yi, Sukyoung K.
Authors
Frazer R. Pearce
Omar Almaini
Alexander Knebe
Violeta Gonzalez-Perez
Andrew Benson
Jeremy Blaizot
Jorge Carretero
Francisco J. Castander
Andrea Cattaneo
Sofía A Cora
Darren J. Croton
Julien E. Devriendt
Fabio Fontanot
Ignacio D. Gargiulo
Will Hartley
Bruno Henriques
Jaehyun Lee
Gary A. Mamon
Julian Onions
Nelson D. Padilla
Chris Power
Chaichalit Srisawat
Adam R.H. Stevens
Peter A. Thomas
Cristian A. Vega-Martínez
Sukyoung K. Yi
Abstract
We present a comparison of the observed evolving galaxy stellar mass functions with the predictions of eight semi-analytic models and one halo occupation distribution model. While most models are able to fit the data at low redshift, some of them struggle to simultaneously fit observations at high redshift. We separate the galaxies into ‘passive’ and ‘star-forming’ classes and find that several of the models produce too many low-mass star-forming galaxies at high redshift compared to observations, in some cases by nearly a factor of 10 in the redshift range 2.5 < z < 3.0. We also find important differences in the implied mass of the dark matter haloes the galaxies inhabit, by comparing with halo masses inferred from observations. Galaxies at high redshift in the models are in lower mass haloes than suggested by observations, and the star formation efficiency in low-mass haloes is higher than observed. We conclude that many of the models require a physical prescription that acts to dissociate the growth of low-mass galaxies from the growth of their dark matter haloes at high redshift.
Citation
Asquith, R., Pearce, F. R., Almaini, O., Knebe, A., Gonzalez-Perez, V., Benson, A., Blaizot, J., Carretero, J., Castander, F. J., Cattaneo, A., Cora, S. A., Croton, D. J., Devriendt, J. E., Fontanot, F., Gargiulo, I. D., Hartley, W., Henriques, B., Lee, J., Mamon, G. A., Onions, J., …Yi, S. K. (2018). Cosmic CARNage II: the evolution of the galaxy stellar mass functionin observations and galaxy formation models. Monthly Notices of the Royal Astronomical Society, 480(1), 1197-1210. https://doi.org/10.1093/mnras/sty1870
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 9, 2018 |
Online Publication Date | Jul 14, 2018 |
Publication Date | Oct 11, 2018 |
Deposit Date | Sep 13, 2018 |
Publicly Available Date | Sep 13, 2018 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 480 |
Issue | 1 |
Pages | 1197-1210 |
DOI | https://doi.org/10.1093/mnras/sty1870 |
Public URL | https://durham-repository.worktribe.com/output/1320171 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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