activity
20002025
most citedSOLAR: Deep Structured Representations for Model-Based Reinforcement Learning

132 citations · 600 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.CO2025★ 5 cited

Encyclopedia Magneticum: Scaling Relations from Cosmic Dawn to Present Day

Klaus Dolag, Rhea-Silvia Remus, Lucas M. Valenzuela +10

Galaxy and halo scaling relations, connecting a broad range of parameters, are well established from observations. The origin of many of these relations and their scatter is still…

astro-ph.GA2018★ 16 cited

Numerical Models for the Diffuse Ionized Gas in Galaxies. II. Three-dimensional radiative transfer in inhomogeneous interstellar structures as a tool for analyzing the diffuse ionized gas

J. A. Weber, A. W. A. Pauldrach, T. L. Hoffmann

Aims: We systematically explore a plausible subset of the parameter space involving effective temperatures and metallicities of the ionizing stellar sources, the effects of the har…

cs.LG2018★ 132 cited

SOLAR: Deep Structured Representations for Model-Based Reinforcement Learning

Marvin Zhang, Sharad Vikram, Laura Smith +3

Model-based reinforcement learning (RL) has proven to be a data efficient approach for learning control tasks but is difficult to utilize in domains with complex observations such…

astro-ph.GA2017★ 57 cited

The Outer Halos of Very Massive Galaxies: BCGs and their DSC in the Magneticum Simulations

Rhea-Silvia Remus, Klaus Dolag, Tadziu L. Hoffmann

Recent hydrodynamic cosmological simulations cover volumes up to Gpc^3 and resolve halos across a wide range of masses and environments, from massive galaxy clusters down to normal…

astro-ph.SR2017★ 14 cited

Carbon line formation and spectroscopy in O-type stars

Luiz P. Carneiro, J. Puls, T. L. Hoffmann

The determination of chemical abundances constitutes a fundamental requirement for obtaining a complete picture of a star. Particularly in massive stars, CNO abundances are of prim…

astro-ph.SR2016★ 16 cited

Atmospheric NLTE-Models for the Spectroscopic Analysis of Blue Stars with Winds. III. X-ray emission from wind-embedded shocks

Luiz P. Carneiro, J. Puls, J. O. Sundqvist +1

X-rays/EUV radiation emitted from wind-embedded shocks in hot, massive stars can affect the ionization balance in their outer atmospheres, and can be the mechanism responsible for…