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Predictions from our terminal model (iteration ...

Predictions from our terminal model (iteration 40) for the 164,297 K and M stars within ...

Zachary Way et al, The Astronomical Journal 171 4

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Correlation between RUWE and overluminosity. Th...

Correlation between RUWE and overluminosity. The top left panel shows the difference dis...

Zachary Way et al, The Astronomical Journal 171 4

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The AAVSO VSX eclipsing binary catalog is shown...

The AAVSO VSX eclipsing binary catalog is shown in four sets based on whether 1) they we...

Zachary Way et al, The Astronomical Journal 171 4

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Density of the Catalog of Systems and its Gaia ...

Density of the Catalog of Systems and its Gaia CMD. Left panel: density normalized by it...

Zachary Way et al, The Astronomical Journal 171 4

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Overluminosity of the SB 2 binaries from M. Kou...

Overluminosity of the SB 2 binaries from M. Kounkel et al. (2021) shown against the ampl...

Zachary Way et al, The Astronomical Journal 171 4

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Total number of systems identified as a functio...

Total number of systems identified as a function of the number of components N in the sy...

Zachary Way et al, The Astronomical Journal 171 4

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Relationship between the overluminosity and eff...

Relationship between the overluminosity and effective temperature ratio of the ASAS-SN B...

Zachary Way et al, The Astronomical Journal 171 4

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Binary sample identified using the ...

Binary sample identified using the ﹩{\rm{\Delta }}R{V}_{\max }﹩ method. The plots are di...

Zachary Way et al, The Astronomical Journal 171 4

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SB 2 binary catalog from M. Kounkel et al. (202...

SB 2 binary catalog from M. Kounkel et al. (2021). The plots are displayed using the sam...

Zachary Way et al, The Astronomical Journal 171 4

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Results of different RUWE cuts for low-mass sta...

Results of different RUWE cuts for low-mass stars from a simulated set of 200,000 binari...

Zachary Way et al, The Astronomical Journal 171 4

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The strong relationship between the optical pho...

The strong relationship between the optical photometry and spectra for low-mass stars. L...

Zachary Way et al, The Astronomical Journal 171 4

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Winnowing from all stars within 100 pc to the R...

Winnowing from all stars within 100 pc to the Regression Sample in four parts. Top left:...

Zachary Way et al, The Astronomical Journal 171 4

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The progress of our iterative method is shown i...

The progress of our iterative method is shown in two aspects. Left panel: number of star...

Zachary Way et al, The Astronomical Journal 171 4

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Comparison between the predictions from our fir...

Comparison between the predictions from our first HISTGRADIENTBOOSTINGREGRESSOR model an...

Zachary Way et al, The Astronomical Journal 171 4

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Multiplicity fraction of K and M dwarf stars in...

Multiplicity fraction of K and M dwarf stars in the Catalog of Systems. Left panel: Gaia...

Zachary Way et al, The Astronomical Journal 171 4

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Comparison between our multiplicity fraction an...

Comparison between our multiplicity fraction and other work. In black are the total mult...

Zachary Way et al, The Astronomical Journal 171 4

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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: 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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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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