collaborators

5 papers

astro-ph.SR2025

Peakbagging the K2 KEYSTONE sample with PBjam: characterising the individual mode frequencies in solar-like oscillators

George T. Hookway, Martin B. Nielsen, Guy R. Davies +5

The pattern of individual mode frequencies in solar-like oscillators provides valuable insight into their properties and interior structures. The identification and characterisatio…

astro-ph.EP2025

TOI-1438: A rare system with two short-period sub-Neptunes and a tentative long-period Jupiter-like planet orbiting a K0V star

Carina M. Persson, Emil Knudstrup, Ilaria Carleo +44

We present the detection and characterisation of the TOI-1438 multi-planet system discovered by TESS. We collected a series of follow-up observations including high-spectral resolu…

astro-ph.SR2025

Luminaries in the Sky: The TESS Legacy Sample of Bright Stars. I. Asteroseismic detections in naked-eye main-sequence and sub-giant solar-like oscillators

Mikkel N. Lund, Ashley Chontos, Frank Grundahl +7

We aim to detect and characterise solar-like oscillations in bright naked-eye (V<6) main-sequence (MS) and subgiant stars observed by TESS. We seek to expand the current benchmark…

astro-ph.SR2025

Precise Asteroseismic Ages for the Helmi Streams

Christopher J. Lindsay, Marc Hon, J. M. Joel Ong +6

The Helmi streams are remnants of a dwarf galaxy that was accreted by the Milky Way and whose stars now form a distinct kinematic and chemical substructure in the Galactic halo. Pr…

astro-ph.SR2025

Is convective turbulence the only exciting mechanism of global p modes in the Sun?

E. Panetier, R. A. García, S. N. Breton +2

In solar-like oscillators, acoustic waves are excited by turbulent motion in the convective envelope and propagate inward, generating a variety of standing pressure modes. When com…