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Bias of damped Lyman-α systems from their cross-correlation with CMB lensing

Abstract:
We cross-correlate the positions of damped Lyman-α systems (DLAs) and their parent quasar catalog with a convergence map derived from the Planck cosmic microwave background (CMB) temperature data. We make consistent measurements of the lensing signal of both samples in both Fourier and configuration space. By interpreting the excess signal present in the DLA catalog with respect to the parent quasar catalog as caused by the large scale structure traced by DLAs, we are able to infer the bias of these objects: bDLA=2.6±0.9. These results are consistent with previous measurements made in cross-correlation with the Lyman-α forest, although the current noise in the lensing data and the low number density of DLAs limits the constraining power of this measurement. We discuss the robustness of the analysis with respect to a number different systematic effects and forecast prospects of carrying out this measurement with data from future experiments.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1475-7516/2018/04/053

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Publisher:
IOP Publishing
Journal:
Journal of Cosmology and Astroparticle Physics More from this journal
Volume:
2018
Issue:
April 2018
Article number:
053
Publication date:
2018-04-20
Acceptance date:
2018-04-10
DOI:
ISSN:
1475-7516


Keywords:
Pubs id:
pubs:847164
UUID:
uuid:c2edf2ee-44bf-4ee4-aa09-fa6a4c863b32
Local pid:
pubs:847164
Source identifiers:
847164
Deposit date:
2018-05-10

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