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| Autori principali: | , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| Accesso online: | https://arxiv.org/abs/2509.25990 |
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| _version_ | 1866908568630853632 |
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| author | Okura, Yuki Futamase, Toshifumi |
| author_facet | Okura, Yuki Futamase, Toshifumi |
| contents | In this paper, we investigate the impact of higher-order distortions on the precise measurement of weak gravitational lensing shear and flexion. We begin by defining generalized higher-order distortions and outlining methods for measuring them. Then, using several lens models, we examine how these distortions affect shear and flexion measurements. Our results show that neglecting higher-order distortions can introduce systematic errors of a few percent in both shear and flexion measurements, indicating that these effects cannot be ignored. Although the strength of these errors depends on factors such as lensing strength and the size of background sources, we demonstrate that simultaneous measurement of higher-order distortions can reduce the systematic errors to below 1% in most cases. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_25990 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The impact of higher-order distortions on the precise measurement of weak gravitational lensing shear and flexion Okura, Yuki Futamase, Toshifumi Cosmology and Nongalactic Astrophysics In this paper, we investigate the impact of higher-order distortions on the precise measurement of weak gravitational lensing shear and flexion. We begin by defining generalized higher-order distortions and outlining methods for measuring them. Then, using several lens models, we examine how these distortions affect shear and flexion measurements. Our results show that neglecting higher-order distortions can introduce systematic errors of a few percent in both shear and flexion measurements, indicating that these effects cannot be ignored. Although the strength of these errors depends on factors such as lensing strength and the size of background sources, we demonstrate that simultaneous measurement of higher-order distortions can reduce the systematic errors to below 1% in most cases. |
| title | The impact of higher-order distortions on the precise measurement of weak gravitational lensing shear and flexion |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2509.25990 |