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Mass–radius relations used for the 2D prior (L....

Mass–radius relations used for the 2D prior (L. Zeng et al. 2016). The shaded region sho...

Mario Damiano et al, The Astronomical Journal 169 2

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Posterior distribution functions of the Bayesia...

Posterior distribution functions of the Bayesian analysis on the modern Earthlike reflec...

Mario Damiano et al, The Astronomical Journal 169 2

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Simulated spectra and data models for the Moder...

Simulated spectra and data models for the Modern and Archean Earth–like scenarios. The d...

Mario Damiano et al, The Astronomical Journal 169 2

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Posterior distribution functions for planetary ...

Posterior distribution functions for planetary mass, radius, and surface pressure for th...

Mario Damiano et al, The Astronomical Journal 169 2

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Posterior distribution functions for planetary ...

Posterior distribution functions for planetary mass, radius, and surface pressure for th...

Mario Damiano et al, The Astronomical Journal 169 2

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Posterior distribution functions for planetary ...

Posterior distribution functions for planetary mass, radius, and surface pressure for th...

Mario Damiano et al, The Astronomical Journal 169 2

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Posterior distribution functions of the Bayesia...

Posterior distribution functions of the Bayesian analysis on the Archean Earth–like refl...

Mario Damiano et al, The Astronomical Journal 169 2

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Posterior distribution functions for planetary ...

Posterior distribution functions for planetary mass, radius, surface pressure, and parti...

Mario Damiano et al, The Astronomical Journal 169 2

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Posterior distribution functions of the Bayesia...

Posterior distribution functions of the Bayesian analysis on the cloud-free modern Earth...

Mario Damiano et al, The Astronomical Journal 169 2

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Posterior distribution functions for planetary ...

Posterior distribution functions for planetary mass, radius, surface pressure, and parti...

Mario Damiano et al, The Astronomical Journal 169 2

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SNR vs. λ for the modern and Archean Earth scen...

SNR vs. λ for the modern and Archean Earth scenarios. The SNR is set to be 20 at 0.75 μm...

Mario Damiano et al, The Astronomical Journal 169 2

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NIRCam and MIRI spectra (rebinned to a resoluti...

NIRCam and MIRI spectra (rebinned to a resolution λ/Δλ = 400) for all 9 stars in MEAD th...

Marjorie Decleir et al, The Astronomical Journal 169 2

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Silicate feature peak optical depth compared to...

Silicate feature peak optical depth compared to the column densities of Mg, Fe, and O in...

Marjorie Decleir et al, The Astronomical Journal 169 2

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3.4 μm (left) and 6.2 μm (right) hydrocarbon fe...

3.4 μm (left) and 6.2 μm (right) hydrocarbon features, normalized to A(V) for all sightl...

Marjorie Decleir et al, The Astronomical Journal 169 2

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Silicate features, ordered from weakest (bottom...

Silicate features, ordered from weakest (bottom) to strongest (top). The skewed Gaussian...

Marjorie Decleir et al, The Astronomical Journal 169 2

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3 μm feature normalized to A(V) for HD073882 (l...

3 μm feature normalized to A(V) for HD073882 (left) and for the rest of the sample (righ...

Marjorie Decleir et al, The Astronomical Journal 169 2

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Silicate feature properties compared to A(V) an...

Silicate feature properties compared to A(V) and A(1500 Å), with literature measurements...

Marjorie Decleir et al, The Astronomical Journal 169 2

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Peak wavelength, λ0, vs. peak optical depth, τ(...

Peak wavelength, λ0, vs. peak optical depth, τ(λ0), compared to literature measurements ...

Marjorie Decleir et al, The Astronomical Journal 169 2

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Observed correlations between silicate feature ...

Observed correlations between silicate feature properties. The gray data points correspo...

Marjorie Decleir et al, The Astronomical Journal 169 2

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Silicate feature peak optical depth compared to...

Silicate feature peak optical depth compared to hydrogen column densities and molecular ...

Marjorie Decleir et al, The Astronomical Journal 169 2

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Distributions of the members of ASCC 19 and ASC...

Distributions of the members of ASCC 19 and ASCC 21 with an RV-to-error ratio greater th...

Qingshun Hu et al, The Astronomical Journal 169 2

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Radial density profiles of ASCC 19 (left) and A...

Radial density profiles of ASCC 19 (left) and ASCC 21 (right) in 3D spatial space. The s...

Qingshun Hu et al, The Astronomical Journal 169 2

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The 3D projection distribution of the cluster p...

The 3D projection distribution of the cluster pair on X–Y (left), Y–Z (middle), and X–Z ...

Qingshun Hu et al, The Astronomical Journal 169 2

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Left panel: the distribution of the metallicity...

Left panel: the distribution of the metallicity [Fe/H] of the members of ASCC 19, derive...

Qingshun Hu et al, The Astronomical Journal 169 2

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3D spatial structure of the cluster pair (ASCC ...

3D spatial structure of the cluster pair (ASCC 19 and ASCC 21), shown with ellipsoidal c...

Qingshun Hu et al, The Astronomical Journal 169 2

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