. Barbato
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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A. Bonfanti
TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS |
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A. Cumming
The primordial entropy of Jupiter |
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A. F. Krenn
The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS |
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A. Khan
A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes |
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A. Rivoldini
A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes |
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A. Tuson
TESS and CHEOPS discover two warm sub-Neptunes transiting the bright K-dwarf HD 15906 |
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B. M. Morris
Investigating the visible phase-curve variability of 55 Cnc e |
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B.-O. Demory & the CHEOPS Science Team (including J.Venturini)
Investigating the visible phase-curve variability of 55 Cnc e |
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C. Dorn
C. Mordasini
C.Lovis
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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Caroline Dorn
Why do more massive stars host larger planets? |
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D. Gandolfi
TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS |
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D. Gandolfi & the CHEOPS Science Team (including J.Venturini)
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d |
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D. Queloz
D. Ségransan
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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E. A. Meier Valdés
Investigating the visible phase-curve variability of 55 Cnc e |
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E. C. Matthews
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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F. Bouchy
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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F. Masset
The importance of thermal torques on the migration of planets growing by pebble accretion |
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F. Pepe
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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F. Roig
Origin and sustainability of the population of asteroids captured in the exterior resonance 1:2 with Mars |
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G. Chaverot
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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G. Lo Curto
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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H. P. Osborn
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d |
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H.P. Osborn & the CHEOPS Science Team (including J.Venturini)
TESS and CHEOPS discover two warm sub-Neptunes transiting the bright K-dwarf HD 15906 |
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Illaria Pascucci
Why do more massive stars host larger planets? |
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J. A. Patel & the CHEOPS Science Team (including J.Venturini)
The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS |
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J. Cuadra
The importance of thermal torques on the migration of planets growing by pebble accretion |
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J. F. Otegi
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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J. Haldemann
The nature of the radius valley. Hints from formation and evolution models. |
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J. Venturini
J.A. Egger & the CHEOPS Science Team (including J.Venturini)
TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS |
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J.B. Delisle
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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Julia Venturini
Why do more massive stars host larger planets? |
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K. Heng
A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes |
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L. Borsato
A new dynamical modeling of the WASP-47 system with CHEOPS observations |
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L. Mayer
The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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L. Senecal
The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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M. Cretignier
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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M. Ikoma
Critical core mass for enriched envelopes: the role of $H_2O$ condensation |
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M. Lendl
The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS |
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M. Lozovsky
Threshold radii of volatile-rich planets |
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M. M. Miller Bertolami
The importance of thermal torques on the migration of planets growing by pebble accretion |
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M. Marmier
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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M. Mayor
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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M. Miller-Bertolami.
Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario |
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M. P. Ronco
M. Schönbächler
The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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M. Stalport
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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Michael Lozovsky
Why do more massive stars host larger planets? |
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N. Hikel
Bayesian analysis of interiors of HD 219134b, Kepler-10b, Kepler-93b, CoRoT-7b, 55 Cnc e, and HD 97658b using stellar abundance proxies |
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N. Unger
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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N.C. Santos
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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O. M. Guilera
P. Figueira
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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R. Burn
The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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R. Gil-Hutton
Origin and sustainability of the population of asteroids captured in the exterior resonance 1:2 with Mars |
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R. Helled
Ravit Helled
Why do more massive stars host larger planets? |
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Robert Feldmann
Why do more massive stars host larger planets? |
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S. Ataiee
Planet Formation, Migration and Habitability | |
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The formation of Jupiter by hybrid pebble-planetesimal accretion. |
S. P. Quanz
The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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S. Udry
The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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T. Gallardo
Origin and sustainability of the population of asteroids captured in the exterior resonance 1:2 with Mars | |
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How to take into account the relativistic effects in dynamical studies of comets |
T. Zingales & the CHEOPS Science Team (including J.Venturini)
A new dynamical modeling of the WASP-47 system with CHEOPS observations |
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V. Nascimbeni
A new dynamical modeling of the WASP-47 system with CHEOPS observations |
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W. Benz
Y. Alibert
Z. Garai
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d |
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Z. Sándor
Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario |
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