Impact of Starlink constellation on Early LSST: a Photometric Analysis of Satellite Trails with BRDF Model

Fuente: arXiv
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Main Author: Lu, Yao
Format: Preprint
Published: 2024
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author Lu, Yao
author_facet Lu, Yao
contents We report a simulation and quantification of the impact of the Starlink constellation on LSST in terms of the trail surface brightness using a BRDF-based satellite photometric model. A total of 11,908 satellites from the Gen1 and Gen2A constellations are used to focus on the interference to the initial phase of LSST operation. The all-sky simulation shows that approximately 69.33% of the visible satellites over station have an apparent brightness greater than 7 mag with a v1.5 satellite model. The impact of satellite streaks exhibit a non-monotonic relationship to the solar altitude, with the worst moments occurring around $-15^{\circ}$ solar altitude. The assessment based on simulated schedules indicates that no trails can reach the saturation-level magnitude, but 71.61% trails show a surface brightness brighter than the best-case crosstalk correctable limits, and this percentage increases as the dodging weight increases. Therefore, avoiding satellites in the scheduler algorithm is an effective mitigation method, but both the number of streaks and their brightness should be taken into account simultaneously.
format Preprint
id arxiv_https___arxiv_org_abs_2403_11118
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Impact of Starlink constellation on Early LSST: a Photometric Analysis of Satellite Trails with BRDF Model
Lu, Yao
Instrumentation and Methods for Astrophysics
We report a simulation and quantification of the impact of the Starlink constellation on LSST in terms of the trail surface brightness using a BRDF-based satellite photometric model. A total of 11,908 satellites from the Gen1 and Gen2A constellations are used to focus on the interference to the initial phase of LSST operation. The all-sky simulation shows that approximately 69.33% of the visible satellites over station have an apparent brightness greater than 7 mag with a v1.5 satellite model. The impact of satellite streaks exhibit a non-monotonic relationship to the solar altitude, with the worst moments occurring around $-15^{\circ}$ solar altitude. The assessment based on simulated schedules indicates that no trails can reach the saturation-level magnitude, but 71.61% trails show a surface brightness brighter than the best-case crosstalk correctable limits, and this percentage increases as the dodging weight increases. Therefore, avoiding satellites in the scheduler algorithm is an effective mitigation method, but both the number of streaks and their brightness should be taken into account simultaneously.
title Impact of Starlink constellation on Early LSST: a Photometric Analysis of Satellite Trails with BRDF Model
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2403.11118