| A chemical survey of exoplanets with ARIEL G Tinetti, P Drossart, P Eccleston, P Hartogh, A Heske, J Leconte, ... Experimental astronomy 46, 135-209, 2018 | 388 | 2018 |
| Jupiter’s evolution with primordial composition gradients A Vazan, R Helled, T Guillot Astronomy & Astrophysics 610, L14, 2018 | 100 | 2018 |
| How cores grow by pebble accretion-I. Direct core growth MG Brouwers, A Vazan, CW Ormel Astronomy & Astrophysics 611, A65, 2018 | 82 | 2018 |
| The evolution and internal structure of Jupiter and Saturn with compositional gradients A Vazan, R Helled, M Podolak, A Kovetz The Astrophysical Journal 829 (2), 118, 2016 | 81 | 2016 |
| The effect of composition on the evolution of giant and intermediate-mass planets A Vazan, A Kovetz, M Podolak, R Helled Monthly Notices of the Royal Astronomical Society 434 (4), 3283-3292, 2013 | 79 | 2013 |
| Equatorial retrograde flow in WASP-43b elicited by deep wind jets? L Carone, R Baeyens, P Mollière, P Barth, A Vazan, L Decin, P Sarkis, ... Monthly Notices of the Royal Astronomical Society 496 (3), 3582-3614, 2020 | 71 | 2020 |
| Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets J Drazkowska, B Bitsch, M Lambrechts, GD Mulders, D Harsono, A Vazan, ... arXiv preprint arXiv:2203.09759, 2022 | 70 | 2022 |
| Convection and mixing in giant planet evolution A Vazan, R Helled, A Kovetz, M Podolak The Astrophysical Journal 803 (1), 32, 2015 | 64 | 2015 |
| Explaining the low luminosity of Uranus: a self-consistent thermal and structural evolution A Vazan, R Helled Astronomy & Astrophysics 633, A50, 2020 | 57 | 2020 |
| How planets grow by pebble accretion-II. Analytical calculations on the evolution of polluted envelopes MG Brouwers, CW Ormel Astronomy & Astrophysics 634, A15, 2020 | 51 | 2020 |
| How planets grow by pebble accretion-III. Emergence of an interior composition gradient CW Ormel, A Vazan, MG Brouwers Astronomy & Astrophysics 647, A175, 2021 | 50 | 2021 |
| A new perspective on the interiors of ice-rich planets: ice–rock mixture instead of ice on top of rock A Vazan, R Sari, R Kessel The Astrophysical Journal 926 (2), 150, 2022 | 40 | 2022 |
| Ariel: Enabling planetary science across light-years G Tinetti, P Eccleston, C Haswell, PO Lagage, J Leconte, T Lüftinger, ... arXiv preprint arXiv:2104.04824, 2021 | 36 | 2021 |
| ON the evolution and survival of protoplanets embedded in a protoplanetary disk A Vazan, R Helled The Astrophysical Journal 756 (1), 90, 2012 | 34 | 2012 |
| Contribution of the core to the thermal evolution of sub-Neptunes A Vazan, CW Ormel, L Noack, C Dominik The Astrophysical Journal 869 (2), 163, 2018 | 30 | 2018 |
| The contribution of the ARIEL space mission to the study of planetary formation D Turrini, Y Miguel, T Zingales, A Piccialli, R Helled, A Vazan, F Oliva, ... Experimental Astronomy 46, 45-65, 2018 | 27 | 2018 |
| TW Hya: an old protoplanetary disc revived by its planet S Nayakshin, T Tsukagoshi, C Hall, A Vazan, R Helled, J Humphries, ... Monthly Notices of the Royal Astronomical Society 495 (1), 285-304, 2020 | 24 | 2020 |
| Exploring the link between star and planet formation with Ariel D Turrini, C Codella, C Danielski, D Fedele, S Fonte, A Garufi, ... Experimental Astronomy, 1-54, 2021 | 22 | 2021 |
| How planets grow by pebble accretion-IV. Envelope opacity trends from sedimenting dust and pebbles MG Brouwers, CW Ormel, A Bonsor, A Vazan Astronomy & Astrophysics 653, A103, 2021 | 22 | 2021 |
| Effect of core cooling on the radius of sub-Neptune planets A Vazan, CW Ormel, C Dominik Astronomy & Astrophysics 610, L1, 2018 | 15 | 2018 |
Ravit HelledDept. of Astrophysics, University of Zurich在 physik.uzh.ch 的电子邮件经过验证
