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Analysis pipeline employed in the present work....

Analysis pipeline employed in the present work. Exoplanet reflectance time series, recor...

Stuart Bartlett et al, The Astronomical Journal 172 1

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Original data related to the radiance of Mars, ...

Original data related to the radiance of Mars, measured in Digital Number. The two verti...

Stuart Bartlett et al, The Astronomical Journal 172 1

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Reflectance converted from data in Figure 2, st...

Reflectance converted from data in Figure 2, still significantly influenced by the phase...

Stuart Bartlett et al, The Astronomical Journal 172 1

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Entropy and compressibility results for Earth a...

Entropy and compressibility results for Earth and Mars reflectance time series at three ...

Stuart Bartlett et al, The Astronomical Journal 172 1

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Results from computational mechanics analysis o...

Results from computational mechanics analysis of Earth and Mars reflectance time series ...

Stuart Bartlett et al, The Astronomical Journal 172 1

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Statistical complexity and entropy rate curves ...

Statistical complexity and entropy rate curves over kernel width parameter values. Earth...

Stuart Bartlett et al, The Astronomical Journal 172 1

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Example time series used in our analysis. The t...

Example time series used in our analysis. The top panel shows the original data for Eart...

Stuart Bartlett et al, The Astronomical Journal 172 1

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The fitting of Martian reflectance as a functio...

The fitting of Martian reflectance as a function of ﹩\cos (\alpha )﹩, where α represents...

Stuart Bartlett et al, The Astronomical Journal 172 1

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Reflectance corrected for phase angle, now infl...

Reflectance corrected for phase angle, now influenced only by variations in surface comp...

Stuart Bartlett et al, The Astronomical Journal 172 1

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Observed RVs and photometric LCs of ET Cru, tog...

Observed RVs and photometric LCs of ET Cru, together with the best-fitting models and co...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Field images of ET Cru from short to long wavel...

Field images of ET Cru from short to long wavelengths: DSS2 Blue (optical), TESS (red op...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Linear and quadratic fits to the O − C residual...

Linear and quadratic fits to the O − C residuals. The far left point belongs to ASAS, wh...

Gökhan Yücel et al, The Astronomical Journal 172 1

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The observed composite spectrum, ϕ = 0.819, of ...

The observed composite spectrum, ϕ = 0.819, of the semidetached binary ET Cru (black) an...

Gökhan Yücel et al, The Astronomical Journal 172 1

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SED of ET Cru constructed from multiwavelength ...

SED of ET Cru constructed from multiwavelength photometric data. Black circles represent...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Determination of the microturbulent velocity (ξ...

Determination of the microturbulent velocity (ξ) for the primary (left panel) and second...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Same as Figure 10, but for the secondary compon...

Same as Figure 10, but for the secondary component. Line profiles are shown for Al III (...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Mesh plots of the binary system ET Cru at orbit...

Mesh plots of the binary system ET Cru at orbital phases 0.75 (left), 0.85 (middle), and...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Selected line profile fits for the ET Cru prima...

Selected line profile fits for the ET Cru primary component from FEROS spectra. Observed...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Comparison of photospheric elemental abundances...

Comparison of photospheric elemental abundances (﹩\mathrm{log}\varepsilon (X)﹩) for the ...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Observations and best-fitting LC and spectrosco...

Observations and best-fitting LC and spectroscopic orbital models for Gaia LCs and FEROS...

Gökhan Yücel et al, The Astronomical Journal 172 1

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The corner plot of the posteriors for the funda...

The corner plot of the posteriors for the fundamental parameters of the components of ET...

Gökhan Yücel et al, The Astronomical Journal 172 1

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TESS LCs of ET Cru obtained in five sectors (11...

TESS LCs of ET Cru obtained in five sectors (11, 37, 38, 64, and 65), with exposure time...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Hα and He I lines at where the spot visibility ...

Hα and He I lines at where the spot visibility is maximum and at the closest orbital pha...

Gökhan Yücel et al, The Astronomical Journal 172 1

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Systematics masquerade as period detections. To...

Systematics masquerade as period detections. Top: the period of the highest peak in the ...

Andrew W. Boyle et al, The Astrophysical Journal Supplement Series 284 2

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Systematics classifier performance vs. rotation...

Systematics classifier performance vs. rotation period. Top left: reliability, defined a...

Andrew W. Boyle et al, The Astrophysical Journal Supplement Series 284 2

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