P. Science

Internal structure of massive terrestrial planets

H. F. Astrophysics, D. Valencia, R. O'Connell, 2005, astro-ph/0511150.

MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis

Tokyo, Auckland, Heidelberg, 2022, 2204.03672.

An eclipsing double-line spectroscopic binary at the stellar/substellar boundary in the Upper Scorpius OB association

Osawa, Tokyo Institute of Technology, Berkeley, 2015, 1511.03083.

Internal structure of massive terrestrial planets

H. F. Astrophysics, D. Valencia, Dimitar D. Sasselov Earth, 2005, astro-ph/0511150.

The Long-Term Evolution of the Atmosphere of Venus: Processes and Feedback Mechanisms

Northern Arizona University, Arizona State University, Tempe, 2022, Space Science Reviews.

Rapid rotation, active nests of convection and global-scale flows in solar-likestars

Boulder, Berkeley, Gif-sur-Yvette., 2007, 0801.1672.

Asymmetric mass ratios for bright double neutron-star mergers

Ny, Cosmology, Bonn, 2020, Nature.

WASP-186 and WASP-187: two hot Jupiters discovered by SuperWASP and SOPHIE with additional observations by TESS

Laboratoire d'Astrophysique de Marseille, Observatoire de Geneve, Observatoire de Haute-Provence, 2020, Monthly Notices of the Royal Astronomical Society.

First detection of acceleration and deceleration in protostellar jets?. Time variability in the Cham

Dublin Institute for Advanced Studies, Centre for Gravitational Astrophysics, L. Tautenburg, 2009, 0906.0561.

Emission line variability of young 10-30 M_Jup companions.I. The case of GQ Lup b and GSC 06214-00210 b

Tx, Austin, Heidelberg, 2023, Astronomy & Astrophysics.

The Co-Ordinated radio and infrared survey for high-mass star formation – V. The CORNISH-South survey and catalogue

Engineering, India., Santiago, 2023, Monthly Notices of the Royal Astronomical Society.

Temperature effects on the 15–85 μm spectra of olivines and pyroxenes

Astronomy, University College London, P. Ade, 2001, astro-ph/0103297.