Designing and conducting experiments are routine practices for modern biologists. The real
challenge, especially in the post-genome era, usually comes not from acquiring data, but …

SUMMARY A major part of organismal complexity and versatility of prokaryotes resides in
their ability to fine-tune gene expression to adequately respond to internal and external …

We present an attempt to reach realistic turbulent regime in direct numerical simulations of
the geodynamo. We rely on a sequence of three convection-driven simulations in a rapidly …

Context. Atmospheric magnetic fields in stars with convective envelopes heat stellar
chromospheres, and thus increase the observed flux in the Ca ii H and K doublet. Starting …

We use the anelastic spherical harmonic code to model the convective dynamo of solar-type
stars. Based on a series of 15 3D MHD simulations spanning four bins in rotation and mass …

Alternative techniques and tools for analyzing biomolecular networks With the recent rapid
advances in molecular biology, high-throughput experimental methods have resulted in …

Despite the lack of a shear-rich tachocline region, low-mass fully convective (FC) stars are
capable of generating strong magnetic fields, indicating that a dynamo mechanism …

The Voyager 2 flybys of Uranus and Neptune revealed the first multipolar planetary
magnetic fields and highlighted how much we have yet to learn about ice giant planets. In …

Cross-validation (CV) is a technique to assess the generalizability of a model to unseen
data. This technique relies on assumptions that may not be satisfied when studying …

We discuss how recent advances in observations, theory and numerical simulations have
allowed the stellar community to progress in its understanding of stellar convection, rotation …