Synthetic spectra tests show Zeeman broadening recovers M dwarf magnetic field strengths more reliably with joint abundance fitting and WAIC selection than with free line strengths or BIC/AIC, which underestimate by 30-50% in active cases.
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NSVS 10653195 is a detached eclipsing binary with two K-type stars of masses 0.6402 and 0.6511 solar masses and radii 0.687 and 0.672 solar radii, showing radius inflation relative to models.
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Testing the reliability of magnetic field strength measurements for M dwarfs
Synthetic spectra tests show Zeeman broadening recovers M dwarf magnetic field strengths more reliably with joint abundance fitting and WAIC selection than with free line strengths or BIC/AIC, which underestimate by 30-50% in active cases.
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Absolute dimensions of the low-mass eclipsing binary system NSVS 10653195
NSVS 10653195 is a detached eclipsing binary with two K-type stars of masses 0.6402 and 0.6511 solar masses and radii 0.687 and 0.672 solar radii, showing radius inflation relative to models.