Edges In Coadded Images
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arXiv
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| Format: | Preprint |
| Veröffentlicht: |
2025
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| _version_ | 1866914576817192960 |
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| author | Sheldon, Erin |
| author_facet | Sheldon, Erin |
| contents | We investigate how discontinuities in the point spread function (PSF) and image noise affect weak gravitational lensing shear measurements. Our focus is on discontinuities that arise in coadded images, particularly when edges from input images cross the coadd region. Using Metacalibration and Metadetection for shear calibration and a simple weighted mean coaddition, we find no significant biases for typical galaxy populations, typical edge hit rates (a few percent), or coadds with tens to hundreds of input images. Biases exceeding requirements for large lensing surveys occur only in extreme conditions: (a) coadds with just two input images; (b) an image edge crosses the object in about 25% of coadds; (c) PSF size variations greater than 25%; (d) relatively small galaxies. Even in these extreme cases, accurate shear recovery is achievable by identifying and removing problematic measurements. We use a simple statistic that quantifies the relative variation in PSF size across each object. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_06929 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Edges In Coadded Images Sheldon, Erin Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics We investigate how discontinuities in the point spread function (PSF) and image noise affect weak gravitational lensing shear measurements. Our focus is on discontinuities that arise in coadded images, particularly when edges from input images cross the coadd region. Using Metacalibration and Metadetection for shear calibration and a simple weighted mean coaddition, we find no significant biases for typical galaxy populations, typical edge hit rates (a few percent), or coadds with tens to hundreds of input images. Biases exceeding requirements for large lensing surveys occur only in extreme conditions: (a) coadds with just two input images; (b) an image edge crosses the object in about 25% of coadds; (c) PSF size variations greater than 25%; (d) relatively small galaxies. Even in these extreme cases, accurate shear recovery is achievable by identifying and removing problematic measurements. We use a simple statistic that quantifies the relative variation in PSF size across each object. |
| title | Edges In Coadded Images |
| topic | Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2509.06929 |