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Effective temperature (Teff) vs. rotation perio...

Effective temperature (Teff) vs. rotation period for ϵ Eri compared to data from three y...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Top: raw coronagraphic image of ϵ Eri from the ...

Top: raw coronagraphic image of ϵ Eri from the observations presented in J. Llop-Sayson ...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Upper limits on the F444W and F210M flux ratio ...

Upper limits on the F444W and F210M flux ratio of ϵ Eri b with respect to the host star ...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Left: comparison between an example Sonora Flam...

Left: comparison between an example Sonora Flame Skimmer model (orange) and a custom PIC...

Aniket Sanghi et al, The Astronomical Journal 171 4

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5σ calibrated contrast curve for F210M (blue) a...

5σ calibrated contrast curve for F210M (blue) and F444W (red) observations of ϵ Eri. The...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Consistency of Sonora Flame Skimmer cloud-free ...

Consistency of Sonora Flame Skimmer cloud-free atmospheric models with NIRCam 5σ upper l...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Top: Sonora Flame Skimmer models for varying me...

Top: Sonora Flame Skimmer models for varying metallicity [M/H] keeping other atmospheric...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Left: the minimum detectable visible reflecting...

Left: the minimum detectable visible reflecting area (AV R) as a function of albedo for ...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Distribution of S/Ns of pixels from the F444W P...

Distribution of S/Ns of pixels from the F444W PSF-subtracted image in a 2 FWHM width ann...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Inferred effective temperature (Teff), bolometr...

Inferred effective temperature (Teff), bolometric luminosity (log Lbol/L⊙), radius, and ...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Predicted F444W magnitude using the clear Sonor...

Predicted F444W magnitude using the clear Sonora Flame Skimmer evolutionary models for t...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Phase angle (blue) and projected separation (re...

Phase angle (blue) and projected separation (red) of ϵ Eri b according to the latest orb...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Reflected light spectra for ϵ Eri b computed wi...

Reflected light spectra for ϵ Eri b computed with PICASO for possible planet radii, atmo...

Aniket Sanghi et al, The Astronomical Journal 171 4

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Top row: calibrated F444W and F210M contrast as...

Top row: calibrated F444W and F210M contrast as a function of KLIP reduction parameters....

Aniket Sanghi et al, The Astronomical Journal 171 4

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Calibrated auroral brightnesses for (a) 557.7 n...

Calibrated auroral brightnesses for (a) 557.7 nm [O I], (b) 630.0 nm [O I], and (c) 636....

Zachariah Milby et al, The Planetary Science Journal 7 3

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Example HIRES data showing the three oxygen emi...

Example HIRES data showing the three oxygen emission lines identified in individual 5-mi...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Three-dimensional projection of Europa’s minimu...

Three-dimensional projection of Europa’s minimum distance from the centrifugal equator. ...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Geometric relationships between the centrifugal...

Geometric relationships between the centrifugal equator of the Jovian plasma sheet and E...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Relative ambient electron density as a function...

Relative ambient electron density as a function of System III east longitude for a plasm...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Best-fit component column densities for (b) mol...

Best-fit component column densities for (b) molecular oxygen (O2) and 1σ detectability t...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Weighted average nightly 630.0 nm [O I] brightn...

Weighted average nightly 630.0 nm [O I] brightness over the five years of observations (...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Fit of the nominal ambient electron density (Fi...

Fit of the nominal ambient electron density (Figure 5) to Europa’s 630.0 nm [O I] bright...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Electron density scale height fits to observati...

Electron density scale height fits to observations of Europa’s 630.0 nm [O I] auroral br...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Correlation between Europa’s normalized 630.0 n...

Correlation between Europa’s normalized 630.0 nm [O I] brightness and distance from the ...

Zachariah Milby et al, The Planetary Science Journal 7 3

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Analysis of four snapshots from the simulation ...

Analysis of four snapshots from the simulation at 4000 K and 75 GPa. The four snapshots ...

Adrien Saurety and Razvan Caracas, The Planetary Science Journal 7 3

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