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We show an adaptation of the silicate index ver...

We show an adaptation of the silicate index versus spectral type (or temperature) as pub...

Emily Calamari et al, The Astrophysical Journal Letters 1000 2

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The top figure shows the planetary-to-protosola...

The top figure shows the planetary-to-protosolar elemental abundance ratio for major vol...

Emily Calamari et al, The Astrophysical Journal Letters 1000 2

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Mg/Si ratios of JWST-observed hot Jupiter host ...

Mg/Si ratios of JWST-observed hot Jupiter host stars vs. separation (semimajor axis). Mg...

Emily Calamari et al, The Astrophysical Journal Letters 1000 2

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Schematic detailing potential atmospheric distr...

Schematic detailing potential atmospheric distributions of silicate cloud species with a...

Emily Calamari et al, The Astrophysical Journal Letters 1000 2

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Comparison of mid-infrared spectra of irradiate...

Comparison of mid-infrared spectra of irradiated exoplanet atmospheres and brown dwarfs....

Emily Calamari et al, The Astrophysical Journal Letters 1000 2

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This figure details how the gaseous Mg/Si ratio...

This figure details how the gaseous Mg/Si ratio changes as a function of the pressure an...

Emily Calamari et al, The Astrophysical Journal Letters 1000 2

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Top panels: the 21 cm power spectrum as a funct...

Top panels: the 21 cm power spectrum as a function of k, for the CDM model (solid), WDM-...

Sudipta Sikder et al, The Astrophysical Journal Letters 1000 2

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Top panels: the 21 cm power spectrum as a funct...

Top panels: the 21 cm power spectrum as a function of z at k = 0.05, 0.1, and 0.5 Mpc−1....

Sudipta Sikder et al, The Astrophysical Journal Letters 1000 2

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Top panels: 21 cm power spectrum as a function ...

Top panels: 21 cm power spectrum as a function of k for the CDM (solid) and large-scale ...

Sudipta Sikder et al, The Astrophysical Journal Letters 1000 2

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Testing convergence with respect to the size of...

Testing convergence with respect to the size of our large-scale grid. We show the 21 cm ...

Sudipta Sikder et al, The Astrophysical Journal Letters 1000 2

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Examples of the dependence of T21 on δ and Vbc ...

Examples of the dependence of T21 on δ and Vbc (each in units of its cosmic standard dev...

Sudipta Sikder et al, The Astrophysical Journal Letters 1000 2

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GEMINI/IGRINS H-band (top) and K-band (bottom) ...

GEMINI/IGRINS H-band (top) and K-band (bottom) IGRINS high-resolution spectrum of the st...

María Laura Arias et al, The Astrophysical Journal Letters 1000 2

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GEMINI/IGRINS observed K-band spectrum of LHA 1...

GEMINI/IGRINS observed K-band spectrum of LHA 115-S 18 (black), with the model composed ...

María Laura Arias et al, The Astrophysical Journal Letters 1000 2

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Different fits for selected portions of LHA 115...

Different fits for selected portions of LHA 115-S 18 K-band spectrum, showing the variat...

María Laura Arias et al, The Astrophysical Journal Letters 1000 2

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Effect of our mass and radius measurement of PS...

Effect of our mass and radius measurement of PSR J0437−4715 on the EOS of high-density m...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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Phase-channel residuals for the best fit to the...

Phase-channel residuals for the best fit to the data of our model with three uniform-tem...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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Spot locations, sizes, and temperatures for the...

Spot locations, sizes, and temperatures for the best fit of our featured model with thre...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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Top: comparison between the bolometric data (hi...

Top: comparison between the bolometric data (histogram) and the best model with three un...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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Mass and radius posteriors, using our best fit ...

Mass and radius posteriors, using our best fit to the data of our model with three unifo...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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Radius posteriors for each of our three models ...

Radius posteriors for each of our three models with a modulated power law (the vertical ...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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Natural log of evidence (top panel) and natural...

Natural log of evidence (top panel) and natural log of maximum likelihood (bottom panel)...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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Contribution of each fit component to the phase...

Contribution of each fit component to the phase-summed count spectrum, as a function of ...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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The same as Figure 8 but for the best three-cir...

The same as Figure 8 but for the best three-circle fit with no modulated power law. Note...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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Waveform after subtraction of the unmodulated b...

Waveform after subtraction of the unmodulated background components (from the 3C50 backg...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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The same as Figure 10 but for the best three-ci...

The same as Figure 10 but for the best three-circle fit that does not include a modulate...

M. C. Miller et al, The Astrophysical Journal Letters 1000 2

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