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V. M. Passegger

1 paper here

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author position
  • last author1

Across the 1 of 1 paper where every author was matched, so the position is known.

fields
  • astro-ph.SR1
ORCID 0000-0002-8569-7243

identity via Semantic Scholar / OpenAlex

most citedGeneralized investigation of the rotation-activity relation: Favouring rotation period instead of Rossby number

210 citations · 210 across the 1 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2022★ 27 cited

A transiting, temperate mini-Neptune orbiting the M dwarf TOI-1759 unveiled by TESS

Néstor Espinoza, Enric Pallé, Jonas Kemmer +66

We report the discovery and characterization of TOI-1759~b, a temperate (400 K) sub-Neptune-sized exoplanet orbiting the M~dwarf TOI-1759 (TIC 408636441). TOI-1759 b was observed b…

astro-ph.EP2022★ 24 cited

Discovery and mass measurement of the hot, transiting, Earth-sized planet GJ 3929 b

J. Kemmer, S. Dreizler, D. Kossakowski +64

We report the discovery of GJ 3929 b, a hot Earth-sized planet orbiting the nearby M3.5 V dwarf star, GJ 3929 (G 180--18, TOI-2013). Joint modelling of photometric observations fro…

astro-ph.SR2014★ 210 cited

Generalized investigation of the rotation-activity relation: Favouring rotation period instead of Rossby number

A. Reiners, M. Schuessler, V. M. Passegger

Magnetic activity in Sun-like and low-mass stars causes X-ray coronal emission, which is stronger for more rapidly rotating stars. This relation is often interpreted in terms of th…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.