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Targets under consideration plotted in the esca...

Targets under consideration plotted in the escape speed–instellation space, in both the ...

Jegug Ih et al, The Astronomical Journal 172 1

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The obtained 95% upper CI as a function of the ...

The obtained 95% upper CI as a function of the total (charged) observing time. Here, the...

Jegug Ih et al, The Astronomical Journal 172 1

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The 80 targets ranked by ESM15 and the bolometr...

The 80 targets ranked by ESM15 and the bolometric priority metric (left), by ESM15 and t...

Jegug Ih et al, The Astronomical Journal 172 1

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The constraints on measured intrinsic probabili...

The constraints on measured intrinsic probability of targets having an atmosphere for su...

Jegug Ih et al, The Astronomical Journal 172 1

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Summary of the population-level injection-recov...

Summary of the population-level injection-recovery simulation. The pessimist hypothesis ...

Jegug Ih et al, The Astronomical Journal 172 1

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The inferred probability of an atmosphere as de...

The inferred probability of an atmosphere as defined in Equation (7) as a function of th...

Jegug Ih et al, The Astronomical Journal 172 1

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The fitness function, −E[ΔBIC], plotted over ge...

The fitness function, −E[ΔBIC], plotted over generations for three different values of p...

Jegug Ih et al, The Astronomical Journal 172 1

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Same as Figure 5, but assuming that the planets...

Same as Figure 5, but assuming that the planets are bare rocks with surfaces of AB = 0.2...

Jegug Ih et al, The Astronomical Journal 172 1

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Cosmic Shoreline for planets—not limited to tra...

Cosmic Shoreline for planets—not limited to transiting rocky planets—around M dwarfs for...

Jegug Ih et al, The Astronomical Journal 172 1

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The optimal set of observations for the disting...

The optimal set of observations for the distinguishing Cosmic Shoreline vs. random hypot...

Jegug Ih et al, The Astronomical Journal 172 1

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Same as Figure 9, but for the Cosmic Shoreline ...

Same as Figure 9, but for the Cosmic Shoreline hypotheses vs. the pessimist hypothesis, ...

Jegug Ih et al, The Astronomical Journal 172 1

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Histogram of ΔBIC values between the Cosmic Sho...

Histogram of ΔBIC values between the Cosmic Shoreline hypothesis and the random hypothes...

Jegug Ih et al, The Astronomical Journal 172 1

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The optimal set of targets for maximizing the Δ...

The optimal set of targets for maximizing the ΔBIC between each Cosmic Shoreline and the...

Jegug Ih et al, The Astronomical Journal 172 1

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Same as Figures 10 and 11, but using the optimi...

Same as Figures 10 and 11, but using the optimized set that maximizes ...

Jegug Ih et al, The Astronomical Journal 172 1

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Same as Figure 10 but between the XUV Cosmic Sh...

Same as Figure 10 but between the XUV Cosmic Shoreline hypothesis and the random hypothe...

Jegug Ih et al, The Astronomical Journal 172 1

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Same as Figure 10 but between the XUV Cosmic Sh...

Same as Figure 10 but between the XUV Cosmic Shoreline and the bolometric Cosmic Shoreli...

Jegug Ih et al, The Astronomical Journal 172 1

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Same as Figure 10 but using the chosen list of ...

Same as Figure 10 but using the chosen list of targets in the Rocky Worlds DDT program.

Jegug Ih et al, The Astronomical Journal 172 1

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Millimeter-level GCRS→BCRS→GCRS frame-closure t...

Millimeter-level GCRS→BCRS→GCRS frame-closure test of the BCRS implementation in JPL Gip...

Slava G. Turyshev et al, The Astronomical Journal 172 1

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RV and photometric observations of TOI-181. In ...

RV and photometric observations of TOI-181. In all cases, the red curves are best-fit mo...

Juan I. Espinoza-Retamal et al, The Astronomical Journal 172 1

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RV and photometric observations of TOI-883. In ...

RV and photometric observations of TOI-883. In all cases, the red curves are best-fit mo...

Juan I. Espinoza-Retamal et al, The Astronomical Journal 172 1

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Mass vs. radius diagram. Gray points are all th...

Mass vs. radius diagram. Gray points are all the transiting exoplanets from TEPCat (J. S...

Juan I. Espinoza-Retamal et al, The Astronomical Journal 172 1

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Orbital period vs. planet radius for transiting...

Orbital period vs. planet radius for transiting planets. Gray points are from the TEPCat...

Juan I. Espinoza-Retamal et al, The Astronomical Journal 172 1

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Stellar obliquity of Neptune (2 ≤ Rp/R⊕ ≤ 6 or ...

Stellar obliquity of Neptune (2 ≤ Rp/R⊕ ≤ 6 or 10 ≤ Mp/M⊕ ≤ 50) and Jupiter (not Neptune...

Juan I. Espinoza-Retamal et al, The Astronomical Journal 172 1

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Inferred stellar obliquity distributions for th...

Inferred stellar obliquity distributions for the samples of Jupiter and Neptune hosts. T...

Juan I. Espinoza-Retamal et al, The Astronomical Journal 172 1

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Inferred stellar obliquity distributions for th...

Inferred stellar obliquity distributions for the different subsamples of Neptune hosts. ...

Juan I. Espinoza-Retamal et al, The Astronomical Journal 172 1

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