activity
20042026
most citedA new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase

1k citations · 3.8k across the 67 of their papers we have counts for

collaborators

68 papers

cs.NE2026

Relocating Nonlinearity: How a Downstream Learner Reshapes What Genetic Programming Must Evolve

Nam H. Le

Genetic programming was conceived as a way of evolving solutions: the program is the answer, and fitness is the error of its own output. A substantial line of work instead makes th…

astro-ph.SR2024

Dimming events of evolved stars due to clouds of molecular gas. Scenarios based on 3D radiation-hydrodynamics simulations with CO5BOLD

Bernd Freytag, Susanne Höfner, Bernhard Aringer +1

The dramatic dimming episode of the red supergiant Betelgeuse in 2019/2020, caused by a partial darkening of the stellar disk, has highlighted gaps in the understanding of the evol…

astro-ph.SR2023

AESOPUS 2.0: Low-Temperature Opacities with Solid Grains

P. Marigo, P. Woitke, E. Tognelli +3

In this study we compute the equation of state and Rosseland mean opacity from temperatures of T~30000 K down to T~400 K, pushing the capabilities of the AESOPUS code (Marigo et al…

astro-ph.SR2023★ 6 cited

Synthetic photometry for carbon-rich giants. V. Effects of grain-size-dependent dust opacities

Kjell Eriksson, Susanne Höfner, Bernhard Aringer

The properties and the evolution of asymptotic giant branch (AGB) stars are strongly influenced by their mass loss through a stellar wind. This is believed to be caused by radiatio…

astro-ph.IM2022★ 51 cited

JWST MIRI/MRS in-flight absolute flux calibration and tailored fringe correction for unresolved sources

D. Gasman, I. Argyriou, G. C. Sloan +18

The MRS is one of the four observing modes of JWST/MIRI. Using JWST in-flight data of unresolved (point) sources, we can derive the MRS absolute spectral response function (ASRF) s…

astro-ph.SR2022★ 30 cited

Low-Temperature Gas Opacities with AESOPUS 2.0

Paola Marigo, Bernhard Aringer, Leo Girardi +1

This work introduces new low-temperature gas opacities, in the range 3.2 <= log(T/K) <= 4.5, computed with the AESOPUS code under the assumption of thermodynamic equilibrium (Marig…