1 – 15 of 18
- show: 15
- |
- sort: year (new to old)
Close
Embed this list
<iframe src=" "
width=" "
height=" "
allowtransparency="true"
frameborder="0">
</iframe>
- 2024
-
Mark
TOI-2266 b: A keystone super-Earth at the edge of the M dwarf radius valley
(
- Contribution to journal › Article
-
Mark
Vapor equilibrium models of accreting rocky planets demonstrate direct core growth by pebble accretion
(
- Contribution to journal › Article
- 2023
-
Mark
Anatomy of rocky planets formed by rapid pebble accretion : II. Differentiation by accretion energy and thermal blanketing
(
- Contribution to journal › Article
-
Mark
Anatomy of rocky planets formed by rapid pebble accretion : III. Partitioning of volatiles between planetary core, mantle, and atmosphere
(
- Contribution to journal › Article
-
Mark
Anatomy of rocky planets formed by rapid pebble accretion : I. How icy pebbles determine the core fraction and FeO contents
(
- Contribution to journal › Article
-
Mark
CHEOPS and TESS view of the ultra-short-period super-Earth TOI-561 b
(
- Contribution to journal › Article
-
Mark
Sublimation of refractory minerals in the gas envelopes of accreting rocky planets
(
- Contribution to journal › Article
- 2022
-
Mark
Nucleation and growth of iron pebbles explains the formation of iron-rich planets akin to Mercury
(
- Contribution to journal › Article
-
Mark
Large Interferometer For Exoplanets (LIFE) : I. Improved exoplanet detection yield estimates for a large mid-infrared space-interferometer mission
(
- Contribution to journal › Article
- 2021
-
Mark
Biosignatures of the Earth : I. Airborne spectropolarimetric detection of photosynthetic life
(
- Contribution to journal › Article
- 2019
-
Mark
Formation of planetary systems by pebble accretion and migration : How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode
(
- Contribution to journal › Article
- 2018
-
Mark
TESS's first planet : A super-Earth transiting the naked-eye star π Mensae
(
- Contribution to journal › Article
- 2017
-
Mark
Planetesimal Formation by the Streaming Instability in a Photoevaporating Disk
(
- Contribution to journal › Article
- 2016
-
Mark
Formation and Early Evolution of Planetary Systems
2016)(
- Thesis › Doctoral thesis (compilation)
-
Mark
Did Jupiter's core form in the innermost parts of the Sun's protoplanetary disc?
(
- Contribution to journal › Article