Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems

A. S. Bonomo, X. Dumusque, A. Massa,A. Mortier, R. Bongiolatti,L. Malavolta,A. Sozzetti,L. A. Buchhave, M. Damasso,R. D. Haywood, A. Morbidelli,D. W. Latham,E. Molinari,F. Pepe,E. Poretti,S. Udry, L. Affer, W. Boschin,D. Charbonneau,R. Cosentino, M. Cretignier,A. Ghedina, E. Lega, M. López-Morales, M. Margini,A. F. Martínez Fiorenzano, M. Mayor,G. Micela, M. Pedani,M. Pinamonti,K. Rice, D. Sasselov, R. Tronsgaard,A. Vanderburg

arxiv(2023)

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摘要
The exoplanet population with orbital periods $P<100$ d around solar-type stars is dominated by super-Earths and sub-Neptunes. These planets are, however, missing in our Solar System, and the reason for that is unknown. Two theoretical scenarios invoke the role of Jupiter as the possible culprit: Jupiter may have acted as a dynamical barrier to the inward migration of sub-Neptunes from beyond the water iceline or, alternatively, may have reduced considerably the inward flux of material (pebbles) required to form super-Earths inside that iceline. Both scenarios predict an anti-correlation between the presence of small planets (SPs) and that of cold Jupiters (CJs) in exoplanetary systems. To test that prediction, we homogeneously analyzed the radial-velocity (RV) measurements of 38 Kepler and K2 transiting SP systems gathered over almost 10 years with the HARPS-N spectrograph, as well as publicly available RVs collected with other facilities. We detected five CJs in three systems, two in Kepler-68, two in Kepler-454, and a very eccentric one in K2-312. We derived an occurrence rate of $9.3^{+7.7}_{-2.9}\%$ for CJs with $0.3-13~M_{Jup}$ and 1-10 au, which is lower but still compatible at $1.3\sigma$ with that measured from RV surveys for solar-type stars, regardless of SP presence. This does not allow us to draw a firm conclusion about the predicted anti-correlation between SPs and CJs, which would require a considerably larger sample. Nevertheless, we found no evidence of previous claims of an excess of CJs in SP systems. As an important by-product of our analyses, we homogeneously determined the masses of 64 Kepler and K2 small planets, reaching a precision better than 5, 7.5 and 10$\sigma$ for 25, 13 and 8 planets, respectively. Finally, we release to the scientific community the 3661 HARPS-N radial velocities used in this work. [Abridged]
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