Roy van Boekel

TL;DR: In this article, the authors apply hydrodynamic evaporation models to different synthetic planet populations that were obtained from a planet formation code based on the core-accretion paradigm.

TL;DR: In this article, a chain of models, linking the formation of a planet to its observable present-day spectrum, is presented, including the planet's formation and migration, its long-term thermodynamic evolution, a variety of disk chemistry models, a non-gray atmospheric model, and a radiometric model to obtain simulated spectroscopic observations.

TL;DR: In this article, scattered light images of the TW Hya disk performed with SPHERE in PDI mode at 063, 079, 124 and 162 micron were presented.

TL;DR: In this article, the properties of irradiated exoplanet atmospheres over a wide parameter range including metallicity, C/O ratio and host spectral type were studied. But the authors performed the calculations with their new Pressure-Temperature Iterator and Spectral Emission Calculator for Planetary Atmospheres (PETIT) code, assuming chemical equilibrium.

TL;DR: In this paper, the authors investigate the young stellar objects (YSOs) in the Lynds 1641 (L1641) cloud using multi-wavelength data including Spitzer, WISE, the Two Micron All Sky Survey, and XMM covering similar to 1390 YSOs across a range of evolutionary stages.