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The stellar-to-halo mass relation of GAMA galaxies from 100 deg2of KiDS weak lensing data

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posted on 2023-06-09, 01:14 authored by Edo van Uitert, Marcello Cacciato, Henk Hoekstra, Margot Brouwer, Cristóbal Sifón, Massimo Viola, Ivan Baldry, Joss Bland-Hawthorn, Sarah Brough, M J I Brown, Ami Choi, Simon P. Driver, Thomas Erben, Catherine Heymans, Hendrik Hildebrandt, Benjamin Joachimi, Konrad Kuijken, Jochen Liske, Jonathan LovedayJonathan Loveday, John McFarland, Lance Miller, Reiko Nakajima, John Peacock, Mario Radovich, A S G Robotham, Peter Schneider, Gert Sikkema, Edward N Taylor, Gijs Verdoes Kleijn
We study the stellar-to-halo mass relation of central galaxies in the range 9.7 < log10(M*/h-2M&sun;) < 11.7 and z < 0.4, obtained from a combined analysis of the Kilo Degree Survey (KiDS) and the Galaxy And Mass Assembly (GAMA) survey. We use ˜100 deg2 of KiDS data to study the lensing signal around galaxies for which spectroscopic redshifts and stellar masses were determined by GAMA. We show that lensing alone results in poor constraints on the stellar-to-halo mass relation due to a degeneracy between the satellite fraction and the halo mass, which is lifted when we simultaneously fit the stellar mass function. At M* > 5 × 1010h-2M&sun;, the stellar mass increases with halo mass as ˜ {}M_h^{0.25}. The ratio of dark matter to stellar mass has a minimum at a halo mass of 8 × 1011h-1M&sun; with a value of M_h/M_*=56_{-10}^{+16} [h]. We also use the GAMA group catalogue to select centrals and satellites in groups with five or more members, which trace regions in space where the local matter density is higher than average, and determine for the first time the stellar-to-halo mass relation in these denser environments. We find no significant differences compared to the relation from the full sample, which suggests that the stellar-to-halo mass relation does not vary strongly with local density. Furthermore, we find that the stellar-to-halo mass relation of central galaxies can also be obtained by modelling the lensing signal and stellar mass function of satellite galaxies only, which shows that the assumptions to model the satellite contribution in the halo model do not significantly bias the stellar-to-halo mass relation. Finally, we show that the combination of weak lensing with the stellar mass function can be used to test the purity of group catalogues.

Funding

Astronomy rolling grant; G0278; STFC-SCIENCE AND TECHNOLOGY FACILITIES COUNCIL; ST/I000976/1

History

Publication status

  • Published

File Version

  • Published version

Journal

Monthly Notices of the Royal Astronomical Society

ISSN

0035-8711

Publisher

Oxford University Press

Issue

3

Volume

459

Page range

3251-3270

Department affiliated with

  • Physics and Astronomy Publications

Full text available

  • Yes

Peer reviewed?

  • Yes

Legacy Posted Date

2016-05-16

First Open Access (FOA) Date

2016-05-16

First Compliant Deposit (FCD) Date

2016-05-13

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