Kavli Affiliate: Aaron Roodman | Summary:The Vera C. Rubin Observatory, with its unprecedented field of view and fast focal ratio, will survey the entire sky every 3.5 nights. This unique capacity requires dealing with off axis light that can produce stray light artefacts on the images. The secondary mirror (M2) baffle restricts the light that […]
Continue.. Modeling of the diffuse background produced by the Vera C. Rubin Observatory M2 baffle scattered light