FLEURY Pierre
Position : Chargé de recherche CNRS
(Supervisor :
LARENA J.)
Visiteur du Institut de Physique Théorique à Gif-sur-Yvette, France
Team: Autre
Other research theme(s) or assignment(s) : - LUPM/Particules, Astroparticules, Cosmologie : Théorie
pierre.fleury
ipht.fr
0614998941
Research Activities: |
Je suis cosmologiste, spécialiste de cosmologie inhomogène et de lentillage gravitationnel. |
Scientific productions :
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Measuring line-of-sight shear with Einstein rings: a proof of concept
Author(s): Hogg N., Fleury P., Larena J., Martinelli Matteo
(Article) Published:
Monthly Notices Of The Royal Astronomical Society, vol. p.5982–6000 (2023)
Links openAccess full text :
Ref Arxiv: 2210.07210
DOI: 10.1093/mnras/stad512
Ref. & Cit.: NASA ADS
Abstract: Line-of-sight effects in strong gravitational lensing have long been treated as a nuisance. However, it was recently proposed that the line-of-sight shear could be a cosmological observable in its own right, if it is not degenerate with lens model parameters. Using the formalism introduced by Fleury et al. (2021a), we firstly demonstrate that the line-of-sight shear can be accurately measured from a simple simulated strong lensing image with percent precision. We then extend our analysis to more complex simulated images and stress test the recovery of the line-of-sight shear when using deficient fitting models, finding that it escapes from degeneracies with lens model parameters, albeit at the expense of the precision. Lastly, we check the validity of the tidal approximation by simulating and fitting an image generated in the presence of many line-of-sight dark matter haloes, finding that an explicit violation of the tidal approximation does not necessarily prevent one from measuring the line-of-sight shear.
Comments: 16 + 3 pages, 14 figures, prepared for submission to MNRAS
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