J/A+A/677/A122ivo://CDS.VizieR/J/A+A/677/A122doi:10.26093/cds/vizier.36770122CDSPinamonti M.Barbato D.Sozzetti A.Affer L.Benatti S.Biazzo K.,Bignamini A.Borsa F.Damasso M.Desidera S.Lanza A.F.Maldonado J.,Mancini L.Naponiello L.Nardiello D.Rainer M.Cabona L.Knapic C.,Andreuzzi G.Cosentino R.Fiorenzano A.Ghedina A.Harutyunyan A.,Lorenzi V.Pedani M.Claudi R.Covino E.Maggio A.Micela G.,Molinari E.Pagano I.Piotto G.Poretti E.2025-02-04T20:00:55Z2023-09-13T08:16:55ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmultiple-starslate-type-starsm-starsspectroscopyexoplanetsradial-velocityvisible-astronomyWith the growth of comparative exoplanetology, it is increasingly clear that the relationship between inner and outer planets plays a key role in unveiling the mechanisms governing formation and evolution models. For this reason, it is important to probe the inner region of systems hosting long-period giants in search of undetected lower mass planetary companions. We aim to present the results of a high-cadence and high-precision radial velocity (RV) monitoring of three late-type dwarf stars hosting long-period giants with well-measured orbits in order to search for short-period sub-Neptunes (SN, Msini<30M_{Earth}_). Building on the results and expertise of our previous studies, we carried out combined fits of our HARPS-N data with literature RVs. We used Markov chain Monte Carlo (MCMC) analyses to refine the literature orbital solutions and search for additional inner planets, applying Gaussian process regression techniques to deal with the stellar activity signals where required. We then used the results of our survey to estimate the frequency of sub-Neptunes in systems hosting cold Jupiters, f(SN|CJ), and compared it with the frequency around field M dwarfs, f(SN). We identify a new short-period, low-mass planet orbiting GJ 328, GJ 328 c, with P_c_=241.8^+1.3^_-1.7_d and M_c_sini=21.4^+3.4^_-3.2_M_{Earth}_. We moreover identify and model the chromospheric activity signals and rotation periods of GJ 649 and GJ 849, around which no additional planet is found. Then, taking into account also planetary system around the previously analysed low-mass star BD-11 4672, we derive an estimate of the frequencies of inner planets in such systems. In particular, f(SN|CJ)=0.25^+0.58^_-0.07_ for mini-Neptunes (10M_{Earth}_<Msini<30M_{Earth}_, P<150d), marginally larger than f(SN). For lower mass planets (Msini<10M_{Earth}_) instead f(SN|CJ)<0.69, which is compatible with f(SN). In light of the newly detected mini-Neptune, we find tentative evidence of a positive correlation between the presence of long-period giant planets and that of inner low-mass planets, f(SN|CJ)>f(SN). This might indicate that cold Jupiters have an opposite influence in the formation of inner sub-Neptunes around late-type dwarfs as opposed to their solar-type counterparts, boosting the formation of mini-Neptunes instead of impeding it.2023A&A...677A.122Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/677/A122CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/677/A122https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/677/A122http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/677/A122https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/677/A122https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/677/A122http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/677/A122GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/677/A122/mjumpObservational HARPS-N dataBJDObservation date (BJD-2400000)dtime.epochdoubleRVRadial Velocitym/sphys.veloc;pos.heliocentricdoublee_RVUncertainty on radial velocitym/sstat.errordoubleCaIIActivity CaII indexspect.indexdoublee_CaIIUncertainty on CaII indexstat.errordoubleHalphaActivity Halpha indexspect.indexdoublee_HalphaUncertainty on Halpha indexstat.error;spect.linedoubleNaIActivity NaI indexmeta.code;spect.indexdoublee_NaIUncertainty on NaI indexstat.errordoubleHeIActivity HeI indexspect.indexdoublee_HeIUncertainty on HeI indexstat.errordoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTargetTarget Identifiermeta.id;meta.mainchar