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Closeby Habitable Exoplanet Survey (CHES). I. Astrometric Noise and Planetary Detection Efficiency Due to Stellar Spots and Faculae
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R. Abuter, A. Amorim, M. Benisty, J. P. Berger, H. Bonnet, G. Bourdarot, P. Bourget, W. Brandner, Y. Clénet, R. Davies, F. Delplancke-Ströbele, R. Dembet, A. Drescher, A. Eckart, F. Eisenhauer, H. Feuchtgruber, G. Finger, N. M. Förster Schreiber, P. Garcia, R. Garcia-Lopez, F. Gao, E. Gendron, R. Genzel, S. Gillessen, M. Hartl, et al. Astronomy & Astrophysics 685 L9 (2024) https://doi.org/10.1051/0004-6361/202449547
The Potential of Detecting Nearby Terrestrial Planets in the HZ with Different Methods
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Activity time series of old stars from late F to early K
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Predictions of Astrometric Jitter for Sun-like Stars. I. The Model and Its Application to the Sun as Seen from the Ecliptic
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Activity time series of old stars from late F to early K
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Gautam Vasisht, Ruslan Belikov, Dan Sirbu, Michael Shao, Charles Beichman, Laura Coyle, Eric Mamajek, Eduardo A. Bendek, Peter Tuthill, Olivier Guyon, Kieran Larkin, Howard A. MacEwen, Makenzie Lystrup, Giovanni G. Fazio, Natalie Batalha, Edward C. Tong and Nicholas Siegler 15 (2018) https://doi.org/10.1117/12.2313919
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High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT)
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Detectability of Earth mass planets with RV techniques around Sun-like stars. The example of the Sun
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