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20232026
most citedAn M dwarf accompanied by a close-in giant orbiter with SPECULOOS

27 citations · 58 across the 10 of their papers we have counts for

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astro-ph.SR2026

Asteroseismology and interferometry of the F7V spectroscopic binary Draconis A in the TESS CVZ

Jonatan Rudrasingam, Mikkel N. Lund, Frank Grundahl +26

We present a detailed analysis of the asteroseismic main-sequence benchmark star Dra A in the TESS northern CVZ. We aim to derive stellar mass and radius from asteroseismic mod…

astro-ph.SR2026

Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES

R. A. García, S. Mathur, G. T. Hookway +31

Solar analogs, stars that closely match the fundamental properties of the Sun, provide key benchmarks for testing stellar structure and evolution across different ages and activity…

astro-ph.SR2026

Asteroseismology of solar-like oscillators: emulating individual mode frequencies with a branching neural network

Owen J. Scutt, Guy R. Davies, Amalie Stokholm +6

Accurately measuring stellar ages and internal structures is challenging, but the inclusion of asteroseismic observables can substantially improve precision. However, the curse of…

astro-ph.SR2025★ 5 cited

Asteroseismology with PBjam 2.0: measuring dipole mode frequencies in coupling regimes from main sequence to low-luminosity red giant stars

M. B. Nielsen, J. M. J. Ong, E. J. Hatt +7

PBjam is an open-source software package for measuring mode frequencies of solar-like oscillators. These frequencies help constrain stellar evolution models to precisely estimate m…

astro-ph.SR2023★ 16 cited

Asteroseismology of Scuti stars: emulating model grids using a neural network

Owen J. Scutt, Simon J. Murphy, Martin B. Nielsen +3

Young Scuti stars have proven to be valuable asteroseismic targets but obtaining robust uncertainties on their inferred properties is challenging. We aim to quantify the random…