Rachel Asquith
Cosmic CARNage II: the evolution of the galaxy stellar mass function in 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
Professor FRAZER PEARCE FRAZER.PEARCE@NOTTINGHAM.AC.UK
PROFESSOR OF PHYSICS
Professor OMAR ALMAINI omar.almaini@nottingham.ac.uk
PROFESSOR OF ASTROPHYSICS
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 function in 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 | Jul 17, 2018 |
Publicly Available Date | Jul 17, 2018 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 480 |
Issue | 1 |
Pages | 1197–1210 |
DOI | https://doi.org/10.1093/mnras/sty1870 |
Keywords | methods:numerical, galaxies:haloes, galaxies: evolution, cosmology:theory, dark matter |
Public URL | https://nottingham-repository.worktribe.com/output/946730 |
Publisher URL | https://academic.oup.com/mnras/article/480/1/1197/5054051 |
Contract Date | Jul 17, 2018 |
Files
sty1870.pdf
(1.1 Mb)
PDF
Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf
You might also like
Increasing AGN sample completeness using long-term near-infrared variability
(2024)
Journal Article
Correcting for the overabundance of low-mass quiescent galaxies in semi-analytic models
(2024)
Journal Article
Downloadable Citations
About Repository@Nottingham
Administrator e-mail: discovery-access-systems@nottingham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search