activity
19972026
most citedEvolution of asymptotic giant branch stars II. Optical to far-infrared isochrones with improved TP-AGB models

1.5k citations · 12.6k across the 179 of their papers we have counts for

collaborators

180 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.GA2023★ 2 cited

Primary Period-Luminosity-Relation Calibrators in the Milky Way: Cepheids and RR Lyrae Physical basis, Calibration, and Applications

Martin Groenewegen

In this invited review I discuss the calibration and applications of the period-luminosity relation of classical Cepheid and RR Lyrae stars. After a brief introduction, starting wi…

astro-ph.SR2022★ 4 cited

Type II and anomalous Cepheids in the Kepler K2 mission

Monika I. Jurkovic, Emese Plachy, László Molnár +4

We present the results of the analysis of Type II and anomalous Cepheids using the data from the Kepler K2 mission. The precise light curves of these pulsating variable stars are t…

astro-ph.SR2022★ 6 cited

Orbital parallax of binary systems compared to GAIA DR3 and the parallax zero-point offset at bright magnitudes

Martin Groenewegen

(abridged)Multiple systems for which the astrometric and spectroscopic orbit are known offer the unique possibility of determining the distance to these systems directly without an…

astro-ph.GA2022★ 7 cited

The intrinsic reddening of the Magellanic Clouds as traced by background galaxies -- III. The Large Magellanic Cloud

Cameron P. M. Bell, Maria-Rosa L. Cioni, Angus H. Wright +15

We present a map of the total intrinsic reddening across ~90 deg of the Large Magellanic Cloud (LMC) derived using optical (ugriz) and near-infrared (IR; YJKs) spectral energ…

astro-ph.SR2022★ 19 cited

A WISE view on extreme AGB stars

Martin Groenewegen

(abridged) Variability is a key property of stars on the asymptotic giant branch (AGB). Their pulsation period is related to the luminosity and mass-loss rate (MLR) of the star. Lo…