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Data availability across X-ray, EUV, FUV, and N...

Data availability across X-ray, EUV, FUV, and NUV wavelength ranges for ExEP Tier A star...

Sarah Peacock et al, The Astronomical Journal 170 5

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Effective area curves for all observatories use...

Effective area curves for all observatories used in this analysis. Gray bars mark the te...

Sarah Peacock et al, The Astronomical Journal 170 5

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Left chart: distribution of stars by the number...

Left chart: distribution of stars by the number of wavelength bands (X-ray, EUV, FUV, NU...

Sarah Peacock et al, The Astronomical Journal 170 5

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Same as Figure 2, but for ExEP Tier B stars.

Sarah Peacock et al, The Astronomical Journal 170 5

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Demographics of stars with usable-quality obser...

Demographics of stars with usable-quality observations from each observatory, compared t...

Sarah Peacock et al, The Astronomical Journal 170 5

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The same as Figure 7, but showing each observat...

The same as Figure 7, but showing each observatory individually. Top panels: demographic...

Sarah Peacock et al, The Astronomical Journal 170 5

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Top panel: when compared to HST NUV flux measur...

Top panel: when compared to HST NUV flux measurements, the BT-Settl PHOENIX models nearl...

Sarah Peacock et al, The Astronomical Journal 170 5

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PHOENIX model spectra for G, K, and M stars wit...

PHOENIX model spectra for G, K, and M stars with (black) and without (red) extended uppe...

Sarah Peacock et al, The Astronomical Journal 170 5

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Data availability distributions across four wav...

Data availability distributions across four wavelength bands (X-ray, EUV, FUV, NUV) and ...

Sarah Peacock et al, The Astronomical Journal 170 5

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Breakdown of data availability for the target s...

Breakdown of data availability for the target stars by observatory. Each pie chart shows...

Sarah Peacock et al, The Astronomical Journal 170 5

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Same as Figure 10, for eROSITA.

Sarah Peacock et al, The Astronomical Journal 170 5

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Same as Figure 10. Top panels: ROSAT; middle pa...

Same as Figure 10. Top panels: ROSAT; middle panels: Swift; bottom panels: XMM-Newton.

Sarah Peacock et al, The Astronomical Journal 170 5

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Same as Figure 10. Top panels: GALEX; middle pa...

Same as Figure 10. Top panels: GALEX; middle panels: HST; bottom panels: IUE.

Sarah Peacock et al, The Astronomical Journal 170 5

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[Mg/Fe] vs. [Fe/H] for stars that host our rock...

[Mg/Fe] vs. [Fe/H] for stars that host our rocky planet sample, as well as all main-sequ...

Aida Behmard et al, The Astronomical Journal 170 5

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All small (RP ≤ 1.8 R⊕), rocky planets from the...

All small (RP ≤ 1.8 R⊕), rocky planets from the Exoplanet Archive (J. L. Christiansen et...

Aida Behmard et al, The Astronomical Journal 170 5

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Planet bulk density vs. all rocky elements cons...

Planet bulk density vs. all rocky elements considered in our analysis in [X/Fe] form. As...

Aida Behmard et al, The Astronomical Journal 170 5

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Planet bulk density vs. all rocky elements cons...

Planet bulk density vs. all rocky elements considered in our analysis in [X/H] form. Roc...

Aida Behmard et al, The Astronomical Journal 170 5

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Rocky planet densities vs. host star [Mg/Fe] fo...

Rocky planet densities vs. host star [Mg/Fe] for planets hosted by both FGK (circles) an...

Aida Behmard et al, The Astronomical Journal 170 5

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Uncompressed (blue) and bulk (green) rocky plan...

Uncompressed (blue) and bulk (green) rocky planet densities vs. host star [Mg/Fe] for pl...

Aida Behmard et al, The Astronomical Journal 170 5

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Same as Figure 7, but for NGC 5634. As with NGC...

Same as Figure 7, but for NGC 5634. As with NGC 5897 (Figure 8), at the depth of DELVE D...

A. Chiti et al, The Astronomical Journal 170 5

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Same as Figure 7, but for NGC 5897. At the dept...

Same as Figure 7, but for NGC 5897. At the depth of DELVE DR2, our model suggests that t...

A. Chiti et al, The Astronomical Journal 170 5

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Comparison of the Jacobi radius at apocenter an...

Comparison of the Jacobi radius at apocenter and pericenter with each GC’s half-light ra...

A. Chiti et al, The Astronomical Journal 170 5

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Comparison of the Jacobi radius at apocenter an...

Comparison of the Jacobi radius at apocenter and pericenter with each GC’s King limiting...

A. Chiti et al, The Astronomical Journal 170 5

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Top left: a color–magnitude diagram of the 1000...

Top left: a color–magnitude diagram of the 1000 closest stars to the center of Pal 5, af...

A. Chiti et al, The Astronomical Journal 170 5

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A comparison of the observed Pal 5 stream in DE...

A comparison of the observed Pal 5 stream in DELVE DR2 (top panels) with a simulation of...

A. Chiti et al, The Astronomical Journal 170 5

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