2020
DOI: 10.1093/mnras/staa1298
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The impact of light polarization effects on weak lensing systematics

Abstract: A fraction of the light observed from edge-on disc galaxies is polarized due to two physical effects: selective extinction by dust grains aligned with the magnetic field and scattering of the anisotropic starlight field. Since the reflection and transmission coefficients of the reflecting and refracting surfaces in an optical system depend on the polarization of incoming rays, this optical polarization produces both (a) a selection bias in favour of galaxies with specific orientations and (b) a polarization-de… Show more

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Cited by 4 publications
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“…Secondly, there are some regions in space where the incoming light has been polarised by different sources, e.g., galactic foreground dust. Lin et al (2020) studied the impact of light polarisation on weak-lensing systematics for the Roman Space Telescope (Spergel et al, 2015). The study found that the systematics introduced by light polarisation is comparable to the Roman Space Telescope's requirements.…”
Section: Optic-level Contributorsmentioning
confidence: 99%
“…Secondly, there are some regions in space where the incoming light has been polarised by different sources, e.g., galactic foreground dust. Lin et al (2020) studied the impact of light polarisation on weak-lensing systematics for the Roman Space Telescope (Spergel et al, 2015). The study found that the systematics introduced by light polarisation is comparable to the Roman Space Telescope's requirements.…”
Section: Optic-level Contributorsmentioning
confidence: 99%