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20132026
most citedThe GALEX Nearby Young-Star Survey

92 citations · 136 across the 10 of their papers we have counts for

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7 papers · 1 filter

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.SR2025★ 6 cited

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.SR2025★ 1 cited

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.SR2025

The orbital parameters of the binary BLAP HD133729 : advantages of the frequency modulation method

Hiromoto Shibahashi, Donald W. Kurtz, Simon J. Murphy

We derive all the orbital parameters of the blue large-amplitude pulsator (BLAP) in the binary system HD133729 by exploiting the frequency modulation (FM) method, which is based on…

astro-ph.SR2024

Pulsations in binary stars -- a short review

Simon J. Murphy

Asteroseismology has become an indispensable method for measuring stellar ages and radii, while binary systems remain the most prevalent tool for determining stellar masses. The sy…

astro-ph.SR2013★ 92 cited

The GALEX Nearby Young-Star Survey

David R. Rodriguez, B. Zuckerman, Joel H. Kastner +3

We describe a method that exploits data from the GALEX ultraviolet and WISE and 2MASS infrared source catalogs, combined with proper motions and empirical pre-main sequence isochro…