Revisiting the multi-planetary system of the nearby star HD 20794. Confirmation of a low-mass planet in the habitable zone of a nearby G-dwarf
NARI N., DUMUSQUE X., HARA N., SUAREZ MASCAREÑO, CRETIGNIER M. et al.
Astron. & Astrophys.
, in press
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The Search for the Inbetweeners: How packed are TESS planetary systems?
HORNER J., WITTENMYER R., KANE S. & HOLT T.
Astron. J.
, accepted
arxiv
Cold Ocean Planets or Rocky Worlds? Extrasolar Analogs of Our Solar System's Icy Moons
QUICK L., ROBERGE A., TOVAR MENDOZZA G., QUINTANA E. & YOUNGBLOOD A.
AGU Fall Meeting 2023
, P24A-08
ADS
VLT/SPHERE robust astrometry of the HR8799 planets at milliarcsecond-level accuracy Orbital architecture analysis with PyAstrOFit
WERTZ O., ABSIL O., GOMEZ GONZALEZ C., MILLI J., GIRARD J. et al.
Astron. & Astrophys.
, 598
, A83
paperarxivADS
Bias and robustness of eccentricity estimates from radial velocity data
HARA N., BOUE G., LASKAR J., DELISLE J. & UNGER N.
MNRAS
, 489
, 738
paperarxiv
A robust, template-free approach to precise radial velocity extraction
RAJPAUL V., AIGRAIN S. & BUCHHAVE L.
MNRAS
, 492
, 3960
paperarxiv
Improving robustness of exoplanetary orbital fits through a regularization of the white and red Doppler noise models. Hints of a 13-year star-spot activity cycle of 55 Cancri