activity
19992025
most citedThe Origin of T Tauri X-ray Emission: New Insights from the Chandra Orion Ultradeep Project

534 citations · 4.4k across the 80 of their papers we have counts for

collaborators

80 papers

astro-ph.SR2025

X-ray activity of nearby G-, K-, and M-type stars and implications for planet habitability around M stars

E. Zhu, T. Preibisch

Context. The intense X-ray and UV emission of some active M stars has raised questions about the habitability of planets around M-type stars. Aims. We aim to determine the unbiased…

astro-ph.SR2023★ 8 cited

The population of young low-mass stars in Trumpler 14

Dominika Itrich, Leonardo Testi, Giacomo Beccari +8

Massive star-forming regions are thought to be the most common birth environments in the Galaxy and the only birth places of very massive stars. Their presence in the stellar clust…

astro-ph.EP2023★ 26 cited

Towards a population synthesis of discs and planets. II. Confronting disc models and observations at the population level

Alexandre Emsenhuber, Remo Burn, Jesse Weder +4

Aims. We want to find the distribution of initial conditions that best reproduces disc observations at the population level. Methods. We first ran a parameter study using a 1D mode…

astro-ph.SR2023

Climbing the Cliffs: Classifying YSOs in the Cosmic Cliffs JWST Data using a Probabilistic Random Forest

B. L. Crompvoets, J. Di Francesco, H. Teimoorinia +1

Among the first observations released to the public from the James Webb Space Telescope (JWST) was a section of the star-forming region NGC 3324 known colloquially as the "Cosmic C…

astro-ph.IM2022★ 16 cited

Twinkle -- a small satellite spectroscopy mission for the next phase of exoplanet science

Ian Stotesbury, Billy Edwards, Jean-Francois Lavigne +35

With a focus on off-the-shelf components, Twinkle is the first in a series of cost competitive small satellites managed and financed by Blue Skies Space Ltd. The satellite is based…

astro-ph.SR2022★ 8 cited

Monitoring accretion rate variability in the Orion Nebula Cluster with the Wendelstein Wide Field Imager

S. Flaischlen, T. Preibisch, M. Kluge +2

The understanding of the accretion process has a central role in the understanding of star and planet formation. We aim to test how accretion variability influences previous correl…