Latest Images
Top: converged temperature profile of the best-...
Top: program-level coadded HST/STIS/E230M spect...
Best-fit model spectrum (gold, T = 13,200 K, ...
Top: raw STIS/E230M white-light curve for KELT-...
Comparison between the Hα observations of F. Ya...
Best-fit sunbather model (gold, T = 13,200 K,...
Same as Figure 3, but for two 1 Å wide bins fro...
χ2/N grids of the mass-loss rate (...
Same as Figure 4, but for two 1 Å wide bins fro...
The initial second-degree systematics vector fi...
Comparison between STIS E230M transit observati...
Collection of exoplanets with measurements of M...
Top: best-fit parent eccentricity distributions...
〈e〉 vs. planet radius bins for the sample of M ...
Left: 〈e〉 vs. adjusted planet radius bin center...
〈e〉 vs. orbital period for planets within three...
Left: 〈e〉 vs. adjusted planet radius radj bin c...
〈e〉 vs. planet radius bin centers for the sampl...
Left: on the top panel, [Fe/H] for single-trans...
Left: e vs. ω posteriors for KOI 247.01 perform...
Top: radius distribution of M dwarf planets in ...
Same as Figure 2, but where 〈e〉 is calculated u...
Left: eccentricity posterior generated by fitti...
Median empirical eccentricity models for planet...
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