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Left: stable orbits are possible for prograde m...

Left: stable orbits are possible for prograde moons located outside the planet’s Roche l...

Emily K. Pass et al, The Astronomical Journal 172 3

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The left plots show the results of our injectio...

The left plots show the results of our injection and recovery test into our JWST observa...

Emily K. Pass et al, The Astronomical Journal 172 3

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Rms residuals of our light-curve fits at differ...

Rms residuals of our light-curve fits at different binning cadences. We analyze the two ...

Emily K. Pass et al, The Astronomical Journal 172 3

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Our NIRISS/SOSS transits of TOI 700 d and e. Un...

Our NIRISS/SOSS transits of TOI 700 d and e. Unbinned data are in gray, binned data are ...

Emily K. Pass et al, The Astronomical Journal 172 3

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We subdivide our light-curve data into five wav...

We subdivide our light-curve data into five wavelength bins, each contributing 20% of th...

Emily K. Pass et al, The Astronomical Journal 172 3

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Morphological changes of the spectral trace dur...

Morphological changes of the spectral trace during our observations, as determined from ...

Emily K. Pass et al, The Astronomical Journal 172 3

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Amplitudes and timescales of the granulation-li...

Amplitudes and timescales of the granulation-like signature observed in main-sequence st...

Emily K. Pass et al, The Astronomical Journal 172 3

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We use the pandora package to illustrate the ef...

We use the pandora package to illustrate the effects of varying moon parameters on the l...

Emily K. Pass et al, The Astronomical Journal 172 3

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Left: a median combination of our observations ...

Left: a median combination of our observations of TOI 700 d (upper panel) and e (lower p...

Emily K. Pass et al, The Astronomical Journal 172 3

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For TOI 700 e, the best-fitting planet-only mod...

For TOI 700 e, the best-fitting planet-only model is shown in black, and the planet+moon...

Emily K. Pass et al, The Astronomical Journal 172 3

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The same as Figure 10, but for the idealized ca...

The same as Figure 10, but for the idealized case where we have removed the correlated n...

Emily K. Pass et al, The Astronomical Journal 172 3

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Retrieved trace abundances for all three retrie...

Retrieved trace abundances for all three retrievals. Each panel shows the posterior dist...

Zoe Ko et al, The Astronomical Journal 172 3

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Posterior distributions for the SC and haze par...

Posterior distributions for the SC and haze parameters across the three retrieval models...

Zoe Ko et al, The Astronomical Journal 172 3

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Retrieved spectra from each retrieval. The soli...

Retrieved spectra from each retrieval. The solid lines represent the median spectrum, an...

Zoe Ko et al, The Astronomical Journal 172 3

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Prior-corrected metallicity and C/O posteriors ...

Prior-corrected metallicity and C/O posteriors for the full-spectrum retrievals, with tr...

Zoe Ko et al, The Astronomical Journal 172 3

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White light-curve fit against data (top panel) ...

White light-curve fit against data (top panel) and residuals (bottom panel).

Zoe Ko et al, The Astronomical Journal 172 3

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Sample wavelength-dependent light-curve fits. T...

Sample wavelength-dependent light-curve fits. There are a total of 441 curves spanning f...

Zoe Ko et al, The Astronomical Journal 172 3

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Comparison between the atmosphere + SC abundanc...

Comparison between the atmosphere + SC abundance posteriors and VULCAN chemical equilibr...

Zoe Ko et al, The Astronomical Journal 172 3

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Chemical equilibrium abundance profiles compute...

Chemical equilibrium abundance profiles computed with VULCAN for TOI-3235 b across metal...

Zoe Ko et al, The Astronomical Journal 172 3

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Three representative cases from our synthetic e...

Three representative cases from our synthetic emission retrieval experiment. The left pa...

Zoe Ko et al, The Astronomical Journal 172 3

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Emission retrieval performance across a grid of...

Emission retrieval performance across a grid of injected atmospheric metallicities and c...

Zoe Ko et al, The Astronomical Journal 172 3

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Posterior distributions from retrieval fitting ...

Posterior distributions from retrieval fitting for the atmospheric model.

Zoe Ko et al, The Astronomical Journal 172 3

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Posterior distributions from retrieval fitting ...

Posterior distributions from retrieval fitting for the atmosphere + SC + GP model.

Zoe Ko et al, The Astronomical Journal 172 3

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Atmosphere + SC retrieval on the full spectrum ...

Atmosphere + SC retrieval on the full spectrum and the truncated spectrum. The left pane...

Zoe Ko et al, The Astronomical Journal 172 3

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Posterior distributions from retrieval fitting ...

Posterior distributions from retrieval fitting for the atmospheric model + SC model.

Zoe Ko et al, The Astronomical Journal 172 3

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ANNOUNCEMENTS

Updated Search and Sort

We have updated the search and sort algorithm to return records in reverse chronological order based on the date/time that the images were uploaded to the Astronomy Image Explorer. This is potentially but rarely different from the publication date. Thank you!