The galaxy-dark matter halo connection: which galaxy properties are correlated with the host halo mass?
Contreras, S.; Baugh, C.M.; Norberg, P.; Padilla, N.
Professor Carlton Baugh email@example.com
Professor Peder Norberg firstname.lastname@example.org
We demonstrate how the properties of a galaxy depend on the mass of its host dark matter subhalo, using two independent models of galaxy formation. For the cases of stellar mass and black hole mass, the median property value displays a monotonic dependence on subhalo mass. The slope of the relation changes for subhalo masses for which heating by active galactic nuclei becomes important. The median property values are predicted to be remarkably similar for central and satellite galaxies. The two models predict considerable scatter around the median property value, though the size of the scatter is model dependent. There is only modest evolution with redshift in the median galaxy property at a fixed subhalo mass. Properties such as cold gas mass and star formation rate, however, are predicted to have a complex dependence on subhalo mass. In these cases, subhalo mass is not a good indicator of the value of the galaxy property. We illustrate how the predictions in the galaxy property–subhalo mass plane differ from the assumptions made in some empirical models of galaxy clustering by reconstructing the model output using a basic subhalo abundance matching scheme. In its simplest form, abundance matching generally does not reproduce the clustering predicted by the models, typically resulting in an overprediction of the clustering signal. Using the predictions of the galaxy formation model for the correlations between pairs of galaxy properties, the basic abundance matching scheme can be extended to reproduce the model predictions more faithfully for a wider range of galaxy properties. Our results have implications for the analysis of galaxy clustering, particularly for low abundance samples.
Contreras, S., Baugh, C., Norberg, P., & Padilla, N. (2015). The galaxy-dark matter halo connection: which galaxy properties are correlated with the host halo mass?. Monthly Notices of the Royal Astronomical Society, 452(2), 1861-1876. https://doi.org/10.1093/mnras/stv1438
|Journal Article Type||Article|
|Acceptance Date||Jun 26, 2015|
|Online Publication Date||Jul 17, 2015|
|Publication Date||Sep 11, 2015|
|Deposit Date||Feb 3, 2016|
|Publicly Available Date||Feb 10, 2016|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publisher||Royal Astronomical Society|
|Peer Reviewed||Peer Reviewed|
|Keywords||Galaxy: evolution, Galaxy: formation, Dark matter, Large-scale structure of Universe.|
Published Journal Article
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2015 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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