Detection Limits of Low-mass, Long-period Exoplanets Using Gaussian Processes Applied to HARPS-N Solar RVs. Langellier, N., Milbourne, T. W., Phillips, D. F., Haywood, R. D., Saar, S. H., Mortier, A., Malavolta, L., Thompson, S., Cameron, A. C., Dumusque, X., Cegla, H. M., Latham, D. W., Maldonado, J., Watson, C. A., Cecconi, M., Charbonneau, D., Cosentino, R., Ghedina, A., Gonzalez, M., Li, C., Lodi, M., López-Morales, M., Micela, G., Molinari, E., Pepe, F., Poretti, E., Rice, K., Sasselov, D., Sozzetti, A., Udry, S., & Walsworth, R. L. arXiv:2008.05970 [astro-ph], August, 2020.
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