2025
Analyzing line-of-sight selection biases in galaxy-scale strong lensing with external convergence and shear
TANG, Xianzhe T. Z.; Simon BIRRER; Anowar J. SHAJIB; Narayan KHADKA; Henry James BEST V et. al.Základní údaje
Originální název
Analyzing line-of-sight selection biases in galaxy-scale strong lensing with external convergence and shear
Autoři
TANG, Xianzhe T. Z.; Simon BIRRER; Anowar J. SHAJIB; Narayan KHADKA a Henry James BEST V
Vydání
Journal of Cosmology and Astroparticle Physics, IOP Publishing Ltd, 2025, 1475-7516
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10308 Astronomy
Stát vydavatele
Velká Británie a Severní Irsko
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Impakt faktor
Impact factor: 5.900 v roce 2024
Organizační jednotka
Přírodovědecká fakulta
UT WoS
001591486200003
EID Scopus
2-s2.0-105019069202
Klíčová slova anglicky
cosmological simulations; gravitational lensing; weak gravitational lensing
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 18. 11. 2025 14:54, Mgr. Marie Novosadová Šípková, DiS.
Anotace
V originále
The upcoming Vera Rubin Observatory Legacy Survey of Space and Time (LSST) will dramatically increase the number of strong gravitational lensing systems, requiring precise modeling of line-of-sight (LOS) effects to mitigate biases in lensing observations and cosmological inferences. We develop a method to construct joint distributions of external convergence (κ ext) and shear (γ ext) for strong lensing LOS by aggregating large-scale structure simulations with high-resolution halo renderings and non-linear correction. Our approach captures both smooth background matter and perturbations from halos, enabling accurate modeling of LOS effects. We apply non-linear LOS corrections to κ ext and γ ext that address the non-additive lensing effects caused by objects along the LOS in strong lensing. We find that, with a minimum image separation of 1.0'', non-linear LOS correction due to the presence of a dominant deflector slightly increases the ratio of quadruple to double lenses; this non-linear LOS correction also introduces systematic biases of ∼ 0.1% for galaxy-AGN lens in the inferred Hubble constant (H 0) if not accounted for. We also observe a 0.66% bias for galaxy-galaxy lenses on H 0, and even larger biases 1.02% for galaxy-AGN systems if LOS effects are not accounted for. These results highlight the importance of LOS for precision cosmology. The publicly available code and datasets provide tools for incorporating LOS effects in future analyses.
Návaznosti
| GM24-10599M, projekt VaV |
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