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Cosmological constraints from galaxy clustering and galaxy–galaxy lensing with extended SubHalo Abundance Matching

Abstract:
We present the first cosmological constraints from a joint analysis of galaxy clustering and galaxy–galaxy lensing using extended SubHalo Abundance Matching (SHAMe). We analyse stellar mass-selected Galaxy And Mass Assembly galaxy clustering and Kilo-Degree Survey (KiDS-1000) galaxy–galaxy lensing and find constraints on , in agreement with Planck at 1.7, with the mass density fluctuation amplitude in 8 sphere at present and the density parameter in total matter. These results are in agreement with the cosmic microwave background results from Planck. We are able to constrain all five SHAMe parameters, which describe the galaxy–subhalo connection. We validate our methodology by first applying it to simulated catalogues, generated from the TNG300 simulation, which mimic the stellar mass selection of our real data. We show that we are able to recover the input cosmology for both our fiducial and all-scale analyses. Our all-scale analysis extends to scales of galaxy–galaxy lensing below , which we exclude in our fiducial analysis to avoid baryonic effects. When including all scales, we find a value of , which is 1.26 higher than our fiducial result (against naive expectations where baryonic feedback should lead to small-scale power suppression), and in agreement with Planck at 0.9. We also find a 21 per cent tighter constraint on and a 29 per cent tighter constraint on compared to our fiducial analysis. This work shows the power and potential of joint small-scale galaxy clustering and galaxy–galaxy lensing analyses using SHAMe.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/staf2143

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author
ORCID:
0000-0002-1220-6028
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Role:
Author
ORCID:
0000-0001-7511-7025
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Role:
Author
ORCID:
0000-0003-2953-3970
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author
More by this author
Role:
Author
ORCID:
0000-0002-7950-6076


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Funder identifier:
https://ror.org/05r0vyz12
More from this funder
Funder identifier:
https://ror.org/057g20z61


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
545
Issue:
4
Pages:
staf2143
Article number:
staf2143
Publication date:
2025-12-04
Acceptance date:
2025-12-01
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
2350853
UUID:
uuid_e085400c-7f3b-4871-ba33-34dcf05ab5e3
Local pid:
pubs:2350853
Source identifiers:
3650262
Deposit date:
2026-01-10
ARK identifier:
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