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Revised figure with corrected calculation of IR...

Revised figure with corrected calculation of IR luminosities.

Clarke J. Esmerian and Nickolay Y. Gnedin, The Astrophysical Journal 965 2

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The spin and orbital evolution for our W-R–BH b...

The spin and orbital evolution for our W-R–BH binaries. All systems have equal mass comp...

Linhao Ma et al, The Astrophysical Journal 965 2

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The dimensionless spin of resulting BHs for our...

The dimensionless spin of resulting BHs for our W-R star models if their masses and angu...

Linhao Ma et al, The Astrophysical Journal 965 2

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The dimensionless spin of resulting BHs for our...

The dimensionless spin of resulting BHs for our W-R star models with the nonlinear dampi...

Linhao Ma et al, The Astrophysical Journal 965 2

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The bias induced by the PSF (shaded regions) re...

The bias induced by the PSF (shaded regions) relative to the PSF correction (dashed line...

Charles E. Romero et al, The Astrophysical Journal 965 2

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The updated (3D) amplitude spectra (top) and ra...

The updated (3D) amplitude spectra (top) and ratio of the two amplitude spectra (bottom)...

Charles E. Romero et al, The Astrophysical Journal 965 2

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Footprints of the images used in our work on 47...

Footprints of the images used in our work on 47 Tucanae. Cyan and azure colors represent...

A. F. Marino et al, The Astrophysical Journal 965 2

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Left: reproduction of the m ...

Left: reproduction of the m F322W2 vs. m F115W...

A. F. Marino et al, The Astrophysical Journal 965 2

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Top: three-color (RGB) image of a portion of th...

Top: three-color (RGB) image of a portion of the studied field of view (field C). We use...

A. F. Marino et al, The Astrophysical Journal 965 2

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Left: m F322W2 vs. m ...

Left: m F322W2 vs. m F150W2 − m ...

A. F. Marino et al, The Astrophysical Journal 965 2

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Top: m F814W vs. C ...

Top: m F814W vs. C F606W,F814W,F322W2 pseudo-C...

A. F. Marino et al, The Astrophysical Journal 965 2

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m F115W vs...

m F115W vs. m F115W − m ...

A. F. Marino et al, The Astrophysical Journal 965 2

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Reproduction of the m F322...

Reproduction of the m F322W2 vs. m F115W − m ...

A. F. Marino et al, The Astrophysical Journal 965 2

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ΔF110W,F160W,F115W,F322W2 vs. ΔF606W,F110W ChM ...

ΔF110W,F160W,F115W,F322W2 vs. ΔF606W,F110W ChM of M dwarfs in field C (panel (a)). Panel...

A. F. Marino et al, The Astrophysical Journal 965 2

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Left: proper motions for stars in field C brigh...

Left: proper motions for stars in field C brighter than m F322W2 = 24....

A. F. Marino et al, The Astrophysical Journal 965 2

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Fraction of 2P stars as a function of the radia...

Fraction of 2P stars as a function of the radial distance from the cluster center. The d...

A. F. Marino et al, The Astrophysical Journal 965 2

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Weighted mean-squared-difference (wMSD) as a fu...

Weighted mean-squared-difference (wMSD) as a function of time using different driving ca...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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Comparison of wMSD for our data-driving algorit...

Comparison of wMSD for our data-driving algorithm vs. linear baseline interpolation algo...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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Comparison of all primitive variables in the in...

Comparison of all primitive variables in the interior of the Data-Driven simulation at a...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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Time–distance plot showing the horizontal expan...

Time–distance plot showing the horizontal expansion of the spheromak along the x-directi...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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Comparison between a potential field extrapolat...

Comparison between a potential field extrapolation (left column), the result of data dri...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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Same as Figure 11, but including field lines in...

Same as Figure 11, but including field lines initiated near the edge of the emerged port...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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Same as Figure 5 but from a top-down perspectiv...

Same as Figure 5 but from a top-down perspective, showing GT (left), Δt = 20δt ...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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Perspective comparison of the GT (left), Δt = 2...

Perspective comparison of the GT (left), Δt = 20δt Data-Driven (middle...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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Schematic diagram of the data-driving algorithm...

Schematic diagram of the data-driving algorithm. The upper row shows several times from ...

Lucas A. Tarr et al, The Astrophysical Journal Supplement Series 270 2

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