LACT array direction reconstruction using 2D Gaussian fits and LightGBM quality weighting achieves sub-0.06 degree angular resolution at 100 TeV, with potential further gains from neural ratio estimation.
Layout optimization and performance of large array of imaging atmo- spheric cherenkov telescope (lact).arXiv preprint arXiv:2409.14382, 2024
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Simulations indicate LACT can reach 5 sigma detection of SS 433 in ~30 hours, spatially separate its jets, and distinguish hadronic components after ~100 hours based on prior LHAASO data.
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Enhancing the Angular Resolution of Large Array of imaging atmospheric Cherenkov Telescope (LACT) at Ultra-High Energies
LACT array direction reconstruction using 2D Gaussian fits and LightGBM quality weighting achieves sub-0.06 degree angular resolution at 100 TeV, with potential further gains from neural ratio estimation.
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Prospects for Observing the Microquasar SS 433 with the LACT Array
Simulations indicate LACT can reach 5 sigma detection of SS 433 in ~30 hours, spatially separate its jets, and distinguish hadronic components after ~100 hours based on prior LHAASO data.