output
19922026
most citedThe SIESTA method for ab initio order-N materials simulation

12k citations

Showing 2021Show all

183 papers · 1 filter

cs.CE2021★ 67 cited

Recurrent Neural Networks (RNNs) with dimensionality reduction and break down in computational mechanics; application to multi-scale localization step

Ling Wu, Ludovic Noels

Artificial Neural Networks (NNWs) are appealing functions to substitute high dimensional and non-linear history-dependent problems in computational mechanics since they offer the p…

astro-ph.HE2021★ 5 cited

The non-thermal emission from the colliding-wind binary Apep

S. del Palacio, P. Benaglia, M. De Becker +2

The recently discovered massive binary system Apep is the most powerful synchrotron emitter among the known Galactic colliding-wind binaries. This makes this particular system of g…

astro-ph.SR2021★ 4 cited

Ultraviolet Spectropolarimetry with Polstar: Clumping and Mass-loss Rate Corrections

Ken Gayley, Jorick S. Vink, Asif ud-Doula +13

The most massive stars are thought to lose a significant fraction of their mass in a steady wind during the main-sequence and blue supergiant phases. This in turn sets the stage fo…

astro-ph.EP2021

BEBOP II: Sensitivity to sub-Saturn circumbinary planets using radial-velocities

Matthew R. Standing, Amaury H. M. J. Triaud, João P. Faria +14

BEBOP is a radial-velocity survey that monitors a sample of single-lined eclipsing binaries, in search of circumbinary planets by using high-resolution spectrographs. Here, we desc…

astro-ph.SR2021★ 14 cited

Dynamical masses for two M1 + mid-M dwarf binaries monitored during the SPHERE-SHINE survey

Beth A. Biller, Antoine Grandjean, Sergio Messina +25

We present orbital fits and dynamical masses for HIP 113201AB and HIP 36985AB, two M1 + mid-M dwarf binary systems monitored as part of the SPHERE SHINE survey. To robustly determi…

astro-ph.SR2021★ 14 cited

Asteroseismology of Cephei stars: The stellar inferences tested in hare and hound exercises

Sébastien Salmon, Patrick Eggenberger, Josefina Montalbán +5

The Cephei pulsators are massive main-sequence stars, presenting low radial-order modes. These modes probe in particular the chemical gradient at the edge of the convective cor…