LIGHTS. The extended point spread functions of the LIGHTS survey at the LBT
With the arrival of the next generation of ultra-deep optical imaging surveys reaching $\mu_V$ $\sim$ 30 mag/arcsec$^2$ (3$\sigma$; 10′′ $\times$ 10′′), the removal of scattered light due to the point spread function (PSF) effect remains a critical step for the scientific exploitation of the low sur...
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| Main Authors: | , , , , , , , , , , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Maynooth Academic Publishing
2025-06-01
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| Series: | The Open Journal of Astrophysics |
| Online Access: | https://doi.org/10.33232/001c.140865 |
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