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Related papers: Three Temperate Neptunes Orbiting Nearby Stars

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We report the discovery of HAT-P-26b, a transiting extrasolar planet orbiting the moderately bright V=11.744 K1 dwarf star GSC 0320-01027, with a period P = 4.234516 +- 0.000015 d, transit epoch Tc = 2455304.65122 +- 0.00035 (BJD), and…

High-precision radial velocity surveys explore the population of low-mass exoplanets orbiting bright stars. This allows accurately deriving their orbital parameters such as their occurrence rate and the statistical distribution of their…

To investigate the origin of the features discovered in the exoplanet population, the knowledge of exoplanets' mass and radius with a good precision is essential. In this paper, we report the discovery of three transiting exoplanets by the…

There are now many known exoplanets with Msin(i) within a factor of two of Neptune's, including the transiting planets GJ436b and HAT-P-11b. Planets in this mass-range are different from their more massive cousins in several ways that are…

Earth and Planetary Astrophysics · Physics 2014-11-20 David S. Spiegel , Adam Burrows , Laurent Ibgui , Ivan Hubeny , John A. Milsom

We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V=11.1 to 12.4) F stars. The planets have periods of P = 2.6940 d to 4.4572 d, masses of 0.60 M_J to 0.80 M_J, and radii of 1.57 R_J to 1.73 R_J.…

We present here the discovery and characterisation of a very light planet around HD4308. The planet orbits its star in 15.56 days. The circular radial-velocity variation presents a tiny semi-amplitude of 4.1 m/s that corresponds to a…

Astrophysics · Physics 2009-11-11 S. Udry , M. Mayor , W. Benz , J. -L. Bertaux , F. Bouchy , C. Lovis , C. Mordasini , F. Pepe , D. Queloz , J. -P. Sivan

Planets with radii between that of the Earth and Neptune (hereafter referred to as sub-Neptunes) are found in close-in orbits around more than half of all Sun-like stars. Yet, their composition, formation, and evolution remain poorly…

Earth and Planetary Astrophysics · Physics 2023-11-30 R. Luque , H. P. Osborn , A. Leleu , E. Pallé , A. Bonfanti , O. Barragán , T. G. Wilson , C. Broeg , A. Collier Cameron , M. Lendl , P. F. L. Maxted , Y. Alibert , D. Gandolfi , J. -B. Delisle , M. J. Hooton , J. A. Egger , G. Nowak , M. Lafarga , D. Rapetti , J. D. Twicken , J. C. Morales , I. Carleo , J. Orell-Miquel , V. Adibekyan , R. Alonso , A. Alqasim , P. J. Amado , D. R. Anderson , G. Anglada-Escudé , T. Bandy , T. Bárczy , D. Barrado Navascues , S. C. C. Barros , W. Baumjohann , D. Bayliss , J. L. Bean , M. Beck , T. Beck , W. Benz , N. Billot , X. Bonfils , L. Borsato , A. W. Boyle , A. Brandeker , E. M. Bryant , J. Cabrera , S. Carrazco Gaxiola , D. Charbonneau , S. Charnoz , D. R. Ciardi , W. D. Cochran , K. A. Collins , I. J. M. Crossfield , Sz. Csizmadia , P. E. Cubillos , F. Dai , M. B. Davies , H. J. Deeg , M. Deleuil , A. Deline , L. Delrez , O. D. S. Demangeon , B. -O. Demory , D. Ehrenreich , A. Erikson , E. Esparza-Borges , B. Falk , A. Fortier , L. Fossati , M. Fridlund , A. Fukui , J. Garcia-Mejia , S. Gill , M. Gillon , E. Goffo , Y. Gomez Maqueo Chew , M. Güdel , E. W. Guenther , M. N. Günther , A. P. Hatzes , Ch. Helling , K. M. Hesse , S. B. Howell , S. Hoyer , K. Ikuta , K. G. Isaak , J. M. Jenkins , T. Kagetani , L. L. Kiss , T. Kodama , J. Korth , K. W. F. Lam , J. Laskar , D. W. Latham , A. Lecavelier des Etangs , J. P. D. Leon , J. H. Livingston , D. Magrin , R. A. Matson , E. C. Matthews , C. Mordasini , M. Mori , M. Moyano , M. Munari , F. Murgas , N. Narita , V. Nascimbeni , G. Olofsson , H. L. M. Osborne , R. Ottensamer , I. Pagano , H. Parviainen , G. Peter , G. Piotto , D. Pollacco , D. Queloz , S. N. Quinn , A. Quirrenbach , R. Ragazzoni , N. Rando , F. Ratti , H. Rauer , S. Redfield , I. Ribas , G. R. Ricker , A. Rudat , L. Sabin , S. Salmon , N. C. Santos , G. Scandariato , N. Schanche , J. E. Schlieder , S. Seager , D. Ségransan , A. Shporer , A. E. Simon , A. M. S. Smith , S. G. Sousa , M. Stalport , Gy. M. Szabó , N. Thomas , A. Tuson , S. Udry , A. M. Vanderburg , V. Van Eylen , V. Van Grootel , J. Venturini , I. Walter , N. A. Walton , N. Watanabe , J. N. Winn , T. Zingales

In 2016, Kepler/K2 detected a system of two sub-Neptunes transiting the star HD 224018, one of them showing a mono-transit event. In 2017, we began a spectroscopic follow-up with HARPS-N to measure the dynamical masses of the planets using…

Context. Low-mass extrasolar planets are presently being discovered at an increased pace by radial velocity and transit surveys, opening a new window on planetary systems. Aims. We are conducting a high-precision radial velocity survey with…

Earth and Planetary Astrophysics · Physics 2015-05-20 C. Lovis , D. Ségransan , M. Mayor , S. Udry , W. Benz , J. -L. Bertaux , F. Bouchy , A. C. M. Correia , J. Laskar , G. Lo Curto , C. Mordasini , F. Pepe , D. Queloz , N. C. Santos

We report the discovery of a Neptune-mass planet around Gl 581 (M3V, M = 0.31 Msol), based on precise Doppler measurements with the HARPS spectrograph at La Silla Observatory. The radial velocities reveal a circular orbit of period P =…

In the favoured core-accretion model of formation of planetary systems, solid planetesimals accumulate to build up planetary cores, which then accrete nebular gas if they are sufficiently massive. Around M-dwarf stars (the most common stars…

One focus of modern astronomy is to detect temperate terrestrial exoplanets well-suited for atmospheric characterisation. A milestone was recently achieved with the detection of three Earth-sized planets transiting (i.e. passing in front…

Gliese 436 is an M dwarf with a mass of 0.45 Msun and hosts the extrasolar planet GL 436b [3, 6, 7, 2], which is currently the least massive transiting planet with a mass of ~23.17 Mearth [10], and the only planet known to transit an M…

Zechmeister et al. (2009) surveyed 38 nearby M dwarfs from March 2000 to March 2007 with VLT2 and the UVES spectrometer. This data has recently been reanalyzed (Butler et al. 2019), yielding a significant improvement in the Doppler velocity…

This paper reports on the detection of a planetary system with three Super-Earths orbiting HD40307. HD40307 is a K2V metal-deficient star at a distance of only 13 parsec, part of the HARPS GTO high-precision planet-search programme. The…

Astrophysics · Physics 2009-11-13 M. Mayor , S. Udry , C. Lovis , F. Pepe , D. Queloz , W. Benz , J. -L. Bertaux , F. Bouchy , C. Mordasini , D. Segransan

HD 191939 (TOI-1339) is a nearby (d=54pc), bright (V=9mag), and inactive Sun-like star (G9 V) known to host a multi-planet transiting system. Ground-based spectroscopic observations confirmed the planetary nature of the three transiting…

Recent observations of giant planets have revealed unexpected bulk densities. Hot Jupiters, in particular, appear larger than expected for their masses compared to planetary evolution models, while warm Jupiters seem denser than expected.…

We report the discovery of two new exoplanet systems around fully convective stars, found from the radial-velocity (RV) variations of their host stars measured with the nIR spectropolarimeter CFHT/SPIRou over multiple years. GJ 3378 b is a…

We report the discovery of a transiting, temperate, Neptune-sized exoplanet orbiting the nearby ($d$ = 27.5 pc), M3V star TOI-1231 (NLTT 24399, L 248-27, 2MASS J10265947-5228099). The planet was detected using photometric data from the…

IW ../submit_V2/abstract.txt ( Row 1 Col 1 6:48 Ctrl-K H for help We report the discovery by the HATSouth network of HATS-7b, a transiting Super-Neptune with a mass of 0.120+/-0.012MJ, a radius of 0.563+/-(0.046,0.034)RJ, and an orbital…