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Light element abundances for the full Sgr sampl...

Light element abundances for the full Sgr sample. Stars in the Sgr streams are marked wi...

Xiaowei Ou et al, The Astronomical Journal 169 5

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Average [α/Fe] vs. [Fe/H] (left), [Sr/Ba] vs. [...

Average [α/Fe] vs. [Fe/H] (left), [Sr/Ba] vs. [Ba/Fe] (middle), and [Ba/Eu] vs. [Ba/H] (...

Xiaowei Ou et al, The Astronomical Journal 169 5

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Neutron-capture elements abundances for the ful...

Neutron-capture elements abundances for the full Sgr sample. Stars in the Sgr streams ar...

Xiaowei Ou et al, The Astronomical Journal 169 5

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Phase space distribution of the Sgr core and st...

Phase space distribution of the Sgr core and stream stars from this study (yellow dots) ...

Xiaowei Ou et al, The Astronomical Journal 169 5

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Fe-peak elements abundances for the full Sgr sa...

Fe-peak elements abundances for the full Sgr sample. Stars in the Sgr streams are marked...

Xiaowei Ou et al, The Astronomical Journal 169 5

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Kiel diagram for the sample with all stars show...

Kiel diagram for the sample with all stars shown in dots. The Dartmouth isochrones are s...

Xiaowei Ou et al, The Astronomical Journal 169 5

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Comparison of means and spreads of various elem...

Comparison of means and spreads of various element abundances of all the stars located i...

Xiaowei Ou et al, The Astronomical Journal 169 5

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Heavy element abundance patterns of six r-I sta...

Heavy element abundance patterns of six r-I stars (Sgr9, Sgr428, Sgr462, Sgr431, Sgr422,...

Xiaowei Ou et al, The Astronomical Journal 169 5

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[Eu/Mg] vs. [Mg/H] for Sgr stars (black open/fi...

[Eu/Mg] vs. [Mg/H] for Sgr stars (black open/filled dots) in comparison with the GSE sta...

Xiaowei Ou et al, The Astronomical Journal 169 5

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PL plots for all ACephs (center (pink) and tail...

PL plots for all ACephs (center (pink) and tail (purple)) in V (left), B (middle), and G...

M. J. Cooke and A. Katherina Vivas, Research Notes of the AAS 9 4

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Left: order 2 white-light-curve fit (0.674–0.85...

Left: order 2 white-light-curve fit (0.674–0.850 μm). Right: light-curve fit for a large...

Kim Morel et al, The Astronomical Journal 169 5

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Results from the principal component analysis o...

Results from the principal component analysis of the calibrated data products (without c...

Kim Morel et al, The Astronomical Journal 169 5

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Top: cross section (column 1300) of the SOSS 2D...

Top: cross section (column 1300) of the SOSS 2D image of the WASP-80 field. The photomet...

Kim Morel et al, The Astronomical Journal 169 5

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Top: raw NIRISS/SOSS order 1 (0.85–2.83 μm) whi...

Top: raw NIRISS/SOSS order 1 (0.85–2.83 μm) white-light curves with 1σ error bars for th...

Kim Morel et al, The Astronomical Journal 169 5

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rms of the residuals from the order 1 white-lig...

rms of the residuals from the order 1 white-light-curve fit (black line) as a function o...

Kim Morel et al, The Astronomical Journal 169 5

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NIRISS/SOSS eclipse spectrum of WASP-80 b accor...

NIRISS/SOSS eclipse spectrum of WASP-80 b according to different modeling approaches. Ea...

Kim Morel et al, The Astronomical Journal 169 5

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Corner plot of the parameters included in the c...

Corner plot of the parameters included in the chemical equilibrium retrieval, except for...

Kim Morel et al, The Astronomical Journal 169 5

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Corner plot of the parameters included in the f...

Corner plot of the parameters included in the free chemistry retrieval, except for the 1...

Kim Morel et al, The Astronomical Journal 169 5

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Data products at several stages of the reductio...

Data products at several stages of the reduction process for the NIRISS/SOSS eclipse obs...

Kim Morel et al, The Astronomical Journal 169 5

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Top: eclipse spectrum of WASP-80 b. The black p...

Top: eclipse spectrum of WASP-80 b. The black points with the 1-σ vertical error bars sh...

Kim Morel et al, The Astronomical Journal 169 5

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Top: median model (blue) along with the 1σ and ...

Top: median model (blue) along with the 1σ and 2σ confidence intervals from the SCARLET ...

Kim Morel et al, The Astronomical Journal 169 5

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Top: raw NIRISS/SOSS order 1 (0.85–2.83 μm) whi...

Top: raw NIRISS/SOSS order 1 (0.85–2.83 μm) white-light curve with 1σ error bars (gray),...

Kim Morel et al, The Astronomical Journal 169 5

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Equilibrium temperature as a function of the Bo...

Equilibrium temperature as a function of the Bond albedo, AB, and the recirculation fact...

Kim Morel et al, The Astronomical Journal 169 5

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Left: median temperature profile from the chemi...

Left: median temperature profile from the chemical equilibrium retrieval, along with its...

Kim Morel et al, The Astronomical Journal 169 5

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Reflected light models of WASP-80 b for a varie...

Reflected light models of WASP-80 b for a variety of cloud species produced with PICASO ...

Kim Morel et al, The Astronomical Journal 169 5

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