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Top: converged temperature profile of the best-...

Top: converged temperature profile of the best-fit Cloudy model to the Mg II feature, wh...

Austin Baldwin et al, The Astronomical Journal 171 3

Top: program-level coadded HST/STIS/E230M spect...

Top: program-level coadded HST/STIS/E230M spectrum of host star KELT-9. Middle: same as ...

Austin Baldwin et al, The Astronomical Journal 171 3

Top: raw STIS/E230M white-light curve for KELT-...

Top: raw STIS/E230M white-light curve for KELT-9b for Visit 1 (left) and Visit 2 (right)...

Austin Baldwin et al, The Astronomical Journal 171 3

Comparison between the Hα observations of F. Ya...

Comparison between the Hα observations of F. Yan & T. Henning (2018), their Gaussian fit...

Austin Baldwin et al, The Astronomical Journal 171 3

Best-fit sunbather model (gold, T  =  13,200 K,...

Best-fit sunbather model (gold, T  =  13,200 K, ﹩\dot{M}\,=\,1{0}^{11.5}﹩ g s−1, Vbroad ...

Austin Baldwin et al, The Astronomical Journal 171 3

Same as Figure 3, but for two 1 Å wide bins fro...

Same as Figure 3, but for two 1 Å wide bins from Visit 1, centered at 2700.2 Å (left) an...

Austin Baldwin et al, The Astronomical Journal 171 3

χ2/N grids of the mass-loss rate (...

χ2/N grids of the mass-loss rate (﹩{\mathrm{log}}_{10}\dot{M}﹩) vs. the broadening veloc...

Austin Baldwin et al, The Astronomical Journal 171 3

Same as Figure 4, but for two 1 Å wide bins fro...

Same as Figure 4, but for two 1 Å wide bins from Visit 2, respectively, outside and insi...

Austin Baldwin et al, The Astronomical Journal 171 3

The initial second-degree systematics vector fi...

The initial second-degree systematics vector fitting for the first transit, with respect...

Austin Baldwin et al, The Astronomical Journal 171 3

Best-fit model spectrum (gold, T  = 13,200 K, ...

Best-fit model spectrum (gold, T  = 13,200 K, ﹩\dot{M}\,=\,1{0}^{12.5}﹩ g s−1, Vbroad = ...

Austin Baldwin et al, The Astronomical Journal 171 3

Comparison between STIS E230M transit observati...

Comparison between STIS E230M transit observations of KELT-9b (blue, purple), WASP-121b ...

Austin Baldwin et al, The Astronomical Journal 171 3

Collection of exoplanets with measurements of M...

Collection of exoplanets with measurements of Mg II in the NUV. The XUV irradiation (90–...

Austin Baldwin et al, The Astronomical Journal 171 3

Top: best-fit parent eccentricity distributions...

Top: best-fit parent eccentricity distributions for the entire sample of singles (green)...

Sheila Sagear et al, The Astronomical Journal 171 2

〈e〉 vs. planet radius bins for the sample of M ...

〈e〉 vs. planet radius bins for the sample of M dwarf planets (red points). The red error...

Sheila Sagear et al, The Astronomical Journal 171 2

Left: 〈e〉 vs. adjusted planet radius bin center...

Left: 〈e〉 vs. adjusted planet radius bin centers for the sample of M dwarf singles in th...

Sheila Sagear et al, The Astronomical Journal 171 2

〈e〉 vs. orbital period for planets within three...

〈e〉 vs. orbital period for planets within three radius bins: 0.5 < Rp < 1.5R⊕ (blue), 1....

Sheila Sagear et al, The Astronomical Journal 171 2

Left: 〈e〉 vs. adjusted planet radius radj bin c...

Left: 〈e〉 vs. adjusted planet radius radj bin centers for singles with 0.5 < radj < 5.1R...

Sheila Sagear et al, The Astronomical Journal 171 2

〈e〉 vs. planet radius bin centers for the sampl...

〈e〉 vs. planet radius bin centers for the sample of M dwarf planets in this work (red po...

Sheila Sagear et al, The Astronomical Journal 171 2

Left: on the top panel, [Fe/H] for single-trans...

Left: on the top panel, [Fe/H] for single-transit planet hosts associated with each adju...

Sheila Sagear et al, The Astronomical Journal 171 2

Left: e vs. ω posteriors for KOI 247.01 perform...

Left: e vs. ω posteriors for KOI 247.01 performed with the method from S23; namely, by d...

Sheila Sagear et al, The Astronomical Journal 171 2

Top: radius distribution of M dwarf planets in ...

Top: radius distribution of M dwarf planets in this sample. Middle: [Fe/H] vs. planet ra...

Sheila Sagear et al, The Astronomical Journal 171 2

Same as Figure 2, but where 〈e〉 is calculated u...

Same as Figure 2, but where 〈e〉 is calculated using the empirical eccentricity model rat...

Sheila Sagear et al, The Astronomical Journal 171 2

Left: eccentricity posterior generated by fitti...

Left: eccentricity posterior generated by fitting the first nine chronological transits ...

Sheila Sagear et al, The Astronomical Journal 171 2

Median empirical eccentricity models for planet...

Median empirical eccentricity models for planets in each of the five radius bins in Tabl...

Sheila Sagear et al, The Astronomical Journal 171 2

KDEs for the planets in each of five radius bins.

KDEs for the planets in each of five radius bins.

Sheila Sagear et al, The Astronomical Journal 171 2

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