collaborators

7 papers

astro-ph.SR2026

Quantifying isochrone-based age uncertainties for rapidly rotating A-type stars

Simon J. Murphy, Anuj Gautam, Zachary R. Claytor

Accurate stellar ages and masses are essential for interpreting the demographics and physical properties of exoplanets, particularly for intermediate-mass, early-type stars where c…

astro-ph.SR2026

Variability classification of TESS targets in LOPS2, the first long-term pointing field of PLATO. Version 1 of the public variability catalogue

Mykyta Kliapets, Pablo Huijse, Jeroen Audenaert +28

The PLAnetary Transits and Oscillations of stars (PLATO) mission is expected to launch in January 2027. A total of 8\% of its data rate will be dedicated to complementary science t…

astro-ph.SR2026

FQ Circini: An Ordinary Nova with a High-mass B1 V(n)(e) Companion Whose Decretion Disk Transfers Mass to the White Dwarf via Roche-Lobe Overflow

Bradley E. Schaefer, Andrew Pearce, Tom Love +4

FQ Cir was an ordinary fast He/N classical nova, peaking at =10.9. The pre-eruption and post-eruption counterpart was at =14.0, making the smallest known classical nova ampli…

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

Asteroseismic detection of a predominantly toroidal magnetic field in the deep interior of the main-sequence F star KIC 9244992

Masao Takata, Simon J. Murphy, Donald W. Kurtz +2

An asteroseismic analysis has revealed a magnetic field in the deep interior of a slowly-rotating main-sequence F star KIC9244992, which was observed by the Kepler spacecraft for f…

astro-ph.EP2025

The Age and High Energy Environment of the Very Young Transiting Exoplanet TOI 1227b

Attila Varga, Joel H. Kastner, Alexander S. Binks +2

The mid-M star TOI~1227 hosts among the youngest known transiting exoplanets. We have conducted new X-ray imaging and optical spectroscopic observations of TOI 1227 aimed at ascert…