activity
20032024
most citedNLTE line formation of Fe for late-type stars. I. Standard stars with 1D and <3D> model atmospheres

356 citations · 5.7k across the 76 of their papers we have counts for

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Showing 2016Show all

10 papers · 1 filter

astro-ph.SR2016

Lower solar atmosphere and magnetism at ultra-high spatial resolution

Remo Collet, Serena Criscuoli, Ilaria Ermolli +8

We present the scientific case for a future space-based telescope aimed at very high spatial and temporal resolution imaging of the solar photosphere and chromosphere. Previous mis…

astro-ph.SR2016★ 41 cited

Non-local thermodynamic equilibrium stellar spectroscopy with 1D and 3D models - II. Chemical properties of the Galactic metal-poor disc and the halo

Maria Bergemann, Remo Collet, Ralph Schoenrich +5

From exploratory studies and theoretical expectations it is known that simplifying approximations in spectroscopic analysis (LTE, 1D) lead to systematic biases of stellar parameter…

astro-ph.SR2016★ 113 cited

Non-local thermodynamic equilibrium stellar spectroscopy with 1D and <3D> models - I. Methods and application to magnesium abundances in standard stars

Maria Bergemann, Remo Collet, Anish M. Amarsi +3

We determine Mg abundances in 6 Gaia benchmark stars using theoretical one-dimensional (1D) hydrostatic model atmospheres, as well as temporally- and spatially-averaged 3D model at…

astro-ph.SR2016★ 42 cited

The asteroseismic surface effect from a grid of 3D convection simulations. I. Frequency shifts from convective expansion of stellar atmospheres

Regner Trampedach, Magnus J. Aarslev, Günter Houdek +4

We analyse the effect on adiabatic stellar oscillation frequencies of replacing the near-surface layers in 1D stellar structure models with averaged 3D stellar surface convection s…

astro-ph.EP2016★ 63 cited

Exoplanetary atmospheric sodium revealed by the orbital motion. Narrow-band transmission spectroscopy of HD 189733b with UVES

S. Khalafinejad, C. von Essen, H. J. Hoeijmakers +8

During primary transits, the spectral signatures of an exoplanet atmosphere can be measured using transmission spectroscopy. The goal of this work is to accurately measure the atom…

astro-ph.EP2016★ 52 cited

Measuring stellar granulation during planet transits

A. Chiavassa, A. Caldas, F. Selsis +6

Stellar activity and convection-related surface structures might cause bias in planet detection and characterization that use these transits. Surface convection simulations help to…