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As for Figure 6, but comparing the two stars in...

As for Figure 6, but comparing the two stars in the Hδ region. The spectrum of ψ Boo has...

Brian D. Mason et al, The Astronomical Journal 170 2

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As for Figure 6, but comparing the two stars in...

As for Figure 6, but comparing the two stars in the near-UV. The spectrum of ψ Boo has b...

Brian D. Mason et al, The Astronomical Journal 170 2

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The new combined orbit solution: plot of relati...

The new combined orbit solution: plot of relative astrometry data for 73 Leo; the X and ...

Brian D. Mason et al, The Astronomical Journal 170 2

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This comparison between 73 Leo (red) and ψ Boo ...

This comparison between 73 Leo (red) and ψ Boo at mid-blue wavelengths. The spectrum of ...

Brian D. Mason et al, The Astronomical Journal 170 2

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Two spectra of 73 Leo, but at different phases ...

Two spectra of 73 Leo, but at different phases (one at the giant’s velocity maximum, the...

Brian D. Mason et al, The Astronomical Journal 170 2

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Radial-velocity data from Table 4, with the new...

Radial-velocity data from Table 4, with the new RV-orbit solution fitted to them. Open t...

Brian D. Mason et al, The Astronomical Journal 170 2

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Plot of measurements for 73 Leo made with the N...

Plot of measurements for 73 Leo made with the NPOI. The ellipse represents the final (i....

Brian D. Mason et al, The Astronomical Journal 170 2

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NPOI measures of the magnitude difference of 73...

NPOI measures of the magnitude difference of 73 Leo. The weighted mean of 3.62(0.06) (P....

Brian D. Mason et al, The Astronomical Journal 170 2

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(Top) Degree of (fractional) radius inflation f...

(Top) Degree of (fractional) radius inflation for our study sample, determined in relati...

Lyra Cao and Keivan G. Stassun, The Astrophysical Journal Letters 988 1

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Magnetic starspot filling fractions as a functi...

Magnetic starspot filling fractions as a function of the rotational Rossby number parame...

Lyra Cao and Keivan G. Stassun, The Astrophysical Journal Letters 988 1

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Direct comparison of the degree of observed rad...

Direct comparison of the degree of observed radius inflation and predictions from the ma...

Lyra Cao and Keivan G. Stassun, The Astrophysical Journal Letters 988 1

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Comparisons of radii and temperatures recovered...

Comparisons of radii and temperatures recovered for individual stars with those predicte...

Lyra Cao and Keivan G. Stassun, The Astrophysical Journal Letters 988 1

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Markov Chain Monte Carlo corner plots showing p...

Markov Chain Monte Carlo corner plots showing parameters recovered for the power-law fit...

Lyra Cao and Keivan G. Stassun, The Astrophysical Journal Letters 988 1

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Binary rejection procedure on the clusters incl...

Binary rejection procedure on the clusters included in this analysis. Marker sizes corre...

Lyra Cao and Keivan G. Stassun, The Astrophysical Journal Letters 988 1

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Markov Chain Monte Carlo corner plots showing p...

Markov Chain Monte Carlo corner plots showing parameters recovered for the linear fit in...

Lyra Cao and Keivan G. Stassun, The Astrophysical Journal Letters 988 1

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The fractional alignment ...

The fractional alignment ﹩{\sigma }_{0}^{2}(\alpha J)﹩ of the lower and highly excited l...

Nataliia G. Shchukina et al, The Astrophysical Journal 988 1

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Electron temperature (left panel) and electron ...

Electron temperature (left panel) and electron density (right panel) as a function of th...

Nataliia G. Shchukina et al, The Astrophysical Journal 988 1

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The fractional alignment ...

The fractional alignment ﹩{\sigma }_{0}^{2}(\alpha J)﹩ of the lower and highly excited l...

Nataliia G. Shchukina et al, The Astrophysical Journal 988 1

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Same as Figure 3, but for the case of observati...

Same as Figure 3, but for the case of observations of a horizontal magnetic field (θB = ...

Nataliia G. Shchukina et al, The Astrophysical Journal 988 1

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Fractional alignment ...

Fractional alignment ﹩{\sigma }_{0}^{2}({\alpha }_{\ell }{J}_{\ell })﹩ of the first ...

Nataliia G. Shchukina et al, The Astrophysical Journal 988 1

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The left and right panels show results for the ...

The left and right panels show results for the Fe X and Fe XIII lines, respectively. Top...

Nataliia G. Shchukina et al, The Astrophysical Journal 988 1

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Same as Figure 2, but for the case of observati...

Same as Figure 2, but for the case of observations of a horizontal magnetic field (θB = ...

Nataliia G. Shchukina et al, The Astrophysical Journal 988 1

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Fourier transforms of the combined ULTRACAM dat...

Fourier transforms of the combined ULTRACAM data set (shown in Figure 2) on WD J0049−252...

Ozcan Caliskan et al, The Astrophysical Journal 988 1

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ULTRACAM light curves of WD J0049−2525 from UT ...

ULTRACAM light curves of WD J0049−2525 from UT 2023 October 5, 6, and 7 (left to right)....

Ozcan Caliskan et al, The Astrophysical Journal 988 1

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Light curves (left panels) and corresponding FT...

Light curves (left panels) and corresponding FTs (right panels) for APO (blue) and Gemin...

Ozcan Caliskan et al, The Astrophysical Journal 988 1

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