A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes C Dorn, J Venturini, A Khan, K Heng, Y Alibert, R Helled, A Rivoldini, ... Astronomy & Astrophysics 597, A37, 2017 | 159 | 2017 |
The nature of the radius valley. Hints from formation and evolution models J Venturini, OM Guilera, J Haldemann, MP Ronco, C Mordasini Astronomy & Astrophysics, Volume 643, id.L1, 10 pp., 2020 | 116 | 2020 |
The nature of the radius valley. Hints from formation and evolution models J Venturini, OM Guilera, J Haldemann, MP Ronco, C Mordasini Astronomy & Astrophysics 643 (id.L1), 10 pp, 2020 | 116 | 2020 |
The formation of Jupiter by hybrid pebble–planetesimal accretion Y Alibert, J Venturini, R Helled, S Ataiee, R Burn, L Senecal, W Benz, ... Nature astronomy 2 (11), 873-877, 2018 | 114 | 2018 |
Planet formation with envelope enrichment: new insights on planetary diversity J Venturini, Y Alibert, W Benz Astronomy & Astrophysics 596, A90, 2016 | 114 | 2016 |
Critical core mass for enriched envelopes: the role of H2O condensation J Venturini, Y Alibert, W Benz, M Ikoma Astronomy & Astrophysics 576, A114, 2015 | 80 | 2015 |
Bayesian analysis of interiors of HD 219134b, Kepler-10b, Kepler-93b, CoRoT-7b, 55 Cnc e, and HD 97658b using stellar abundance proxies C Dorn, NR Hinkel, J Venturini Astronomy & Astrophysics 597, A38, 2017 | 72 | 2017 |
The formation of mini-Neptunes J Venturini, R Helled The Astrophysical Journal 848 (2), 95, 2017 | 65 | 2017 |
Jupiter’s heavy-element enrichment expected from formation models J Venturini, R Helled Astronomy & Astrophysics 634, A31, 2020 | 46 | 2020 |
Giant planet formation at the pressure maxima of protoplanetary disks-II. A hybrid accretion scenario OM Guilera, Z Sándor, MP Ronco, J Venturini, MMM Bertolami Astronomy & Astrophysics 642, A140, 2020 | 41 | 2020 |
Threshold radii of volatile-rich planets M Lozovsky, R Helled, C Dorn, J Venturini The Astrophysical Journal 866 (1), 49, 2018 | 40 | 2018 |
Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses J Venturini, OM Guilera, MP Ronco, C Mordasini Astronomy & Astrophysics 644, A174, 2020 | 38 | 2020 |
Setting the stage: planet formation and volatile delivery J Venturini, MP Ronco, OM Guilera Space Science Reviews 216, 1-32, 2020 | 29 | 2020 |
Using deep neural networks to compute the mass of forming planets Y Alibert, J Venturini Astronomy & Astrophysics 626, A21, 2019 | 27 | 2019 |
The primordial entropy of Jupiter A Cumming, R Helled, J Venturini Monthly Notices of the Royal Astronomical Society 477 (4), 4817-4823, 2018 | 22 | 2018 |
Origin and sustainability of the population of asteroids captured in the exterior resonance 1: 2 with Mars T Gallardo, J Venturini, F Roig, R Gil-Hutton Icarus 214 (2), 632-644, 2011 | 21 | 2011 |
The importance of thermal torques on the migration of planets growing by pebble accretion OM Guilera, MM Miller Bertolami, F Masset, J Cuadra, J Venturini, ... Monthly Notices of the Royal Astronomical Society 507 (3), 3638-3652, 2021 | 15 | 2021 |
TOI-5678b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPS S Ulmer-Moll, HP Osborn, A Tuson, JA Egger, M Lendl, P Maxted, ... Astronomy & Astrophysics 674, A43, 2023 | 12 | 2023 |
The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS AF Krenn, M Lendl, JA Patel, L Carone, M Deleuil, S Sulis, AC Cameron, ... Astronomy & Astrophysics 672, A24, 2023 | 12 | 2023 |
Why do more massive stars host larger planets? M Lozovsky, R Helled, I Pascucci, C Dorn, J Venturini, R Feldmann Astronomy & Astrophysics 652, A110, 2021 | 10 | 2021 |