collaborators

5 papers

astro-ph.SR2026

Testing the reliability of magnetic field strength measurements for M dwarfs

I. Amateis, O. Kochukhov, A. Hahlin

M dwarfs host strong magnetic fields that can be measured using several complementary techniques. However, the impact of key methodological choices on Zeeman broadening diagnostics…

astro-ph.EP2026

VLT/CRIRES+ observations of warm Neptune WASP-107 b: Challenges in detecting molecules with ground-based transmission spectroscopy of cooler and cloudy exoplanets

Linn Boldt-Christmas, Adam D. Rains, Nikolai Piskunov +15

Atmospheres of transiting exoplanets can be studied spectroscopically using space-based or ground-based observations. Each has its own strengths and weaknesses, so there are benefi…

astro-ph.EP2026

Cloudy with a chance of metals: Indications of CO in the atmosphere of GJ 1214 b from high-resolution K-band spectroscopy

L. Nortmann, D. Cont, F. Lesjak +13

Sub-Neptune exoplanets frequently exhibit muted transmission spectra, with GJ 1214 b being the most prominent example. Following years of intense observing campaigns yielding featu…

astro-ph.IM2026

Detached eclipsing binary star science in the 2040s

Pierre F. L. Maxted, Dominic M. Bowman, Thomas G. Wilson +7

Detached eclipsing binary stars (DEBS) are currently the best source of accurate and precise fundamental stellar parameters. This makes DEBS crucial targets for constraining the im…

astro-ph.SR2025

Fundamental effective temperature measurements for eclipsing binary stars - VII. The solar twin in LL Aquarii

N. J. Miller, P. F. L. Maxted, A. Hahlin +1

The eclipsing binary LL Aqr is a bright V = 9.32, detached system consisting of two solar-type stars in an eccentric orbit (P = 20.2 d). The secondary component, LL Aqr B, was prev…