Detection Limits of Low-mass, Long-period Exoplanets Using Gaussian Processes Applied to HARPS-N Solar Radial Velocities. 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., Buchschacher, N., 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. The Astronomical Journal, 161(6):287, American Astronomical Society, may, 2021.
Detection Limits of Low-mass, Long-period Exoplanets Using Gaussian Processes Applied to HARPS-N Solar Radial Velocities [pdf]Pdf  Detection Limits of Low-mass, Long-period Exoplanets Using Gaussian Processes Applied to HARPS-N Solar Radial Velocities [link]Link  doi  bibtex   4 downloads  

Downloads: 4