A. Bonfanti
| Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valley |
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A. Cumming
| The primordial entropy of Jupiter |
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A. Emsenhuber
| The PAIRS project: a global formation model for planets in binaries. I. Effect of disc truncation on the growth of S-type planets |
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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. Leleu
| A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 |
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A. Nigioni
| Mind the companion: Demographics of transiting S-type exoplanets | |
|---|---|
| The PAIRS project: a global formation model for planets in binaries. I. Effect of disc truncation on the growth of S-type planets |
A. Rivoldini
| A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes |
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Alexandre Emsenhuber
Arianna Nigioni
| The PAIRS project: a global formation model for planets in binaries. II. Gravitational perturbation effects from secondary stars |
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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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CHEOPS Science Team
| Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valley |
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CHEOPS Science Team (including J.Venturini)
| A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 |
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Christoph Mordasini
| A radius valley between migrated steam worlds and evaporated rocky cores |
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D. Barbato
| The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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D. Queloz
| The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
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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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Diego Turrini
| The PAIRS project: a global formation model for planets in binaries. II. Gravitational perturbation effects from secondary stars |
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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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Emeline Bolmont
| The PAIRS project: a global formation model for planets in binaries. II. Gravitational perturbation effects from secondary stars |
|---|
F. Bouchy
F. Masset
| The importance of thermal torques on the migration of planets growing by pebble accretion |
|---|
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 |
|---|
H. P. Osborn
| A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 |
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I. Pascucci
| Why do more massive stars host larger planets? |
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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
J. Venturini
J.B. Delisle
| The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
|---|
Jonas Haldemann
| A radius valley between migrated steam worlds and evaporated rocky cores |
|---|
Julia Venturini
K. Heng
| A generalized Bayesian inference method for constraining the interiors of super Earths and sub-Neptunes |
|---|
L. Mayer
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
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L. Parc
| Mind the companion: Demographics of transiting S-type exoplanets | |
|---|---|
| From super-Earths to sub-Neptunes: Observational constraints and connections to theoretical models |
L. Senecal
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
|---|
Lina Y. Messamah
| Mind the companion: Demographics of transiting S-type exoplanets |
|---|
Lokesh Mishra
| A radius valley between migrated steam worlds and evaporated rocky cores |
|---|
M. Brady
| Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valley |
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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. Lozovsky
| Why do more massive stars host larger planets? | |
|---|---|
| Threshold radii of volatile-rich planets |
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 |
|---|
M. Miller Bertolami
| A fading radius valley towards M dwarfs, a persistent density valley across stellar types |
|---|
M. Miller-Bertolami.
| Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario |
|---|
M. P. Ronco
M. Schönbächler
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
|---|
M. Stalport
| The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
|---|
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 |
|---|
N. Jungo
| The PAIRS project: a global formation model for planets in binaries. I. Effect of disc truncation on the growth of S-type planets |
|---|
N. Unger
| The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
|---|
N.C. Santos
| The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
|---|
O. M. Guilera
P. Figueira
| The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
|---|
R. Burn
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
|---|
R. Feldmann
| Why do more massive stars host larger planets? |
|---|
R. Gil-Hutton
| Origin and sustainability of the population of asteroids captured in the exterior resonance 1:2 with Mars |
|---|
R. Helled
R. Luque
| A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067 |
|---|
Remo Burn
| A radius valley between migrated steam worlds and evaporated rocky cores |
|---|
S. Ataiee
| Planet Formation, Migration and Habitability | |
|---|---|
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
S. P. Quanz
| The formation of Jupiter by hybrid pebble-planetesimal accretion. |
|---|
S. Udry
| The CORALIE survey for southern extrasolar planets XIX. Brown dwarfs and stellar companions unveiled by radial velocity and astrometry |
|---|
T. G. Wilson
| Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valley |
|---|
T. Gallardo
| Origin and sustainability of the population of asteroids captured in the exterior resonance 1:2 with Mars | |
|---|---|
| How to take into account the relativistic effects in dynamical studies of comets |
W. Benz
Y. Alibert
Yann Alibert
| The PAIRS project: a global formation model for planets in binaries. II. Gravitational perturbation effects from secondary stars |
|---|
Z. Sándor
| Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario |
|---|
and Thomas Henning
| A radius valley between migrated steam worlds and evaporated rocky cores |
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