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Synthetic models associated with the star’s par...

Synthetic models associated with the star’s parameters and default abundances calculated...

Neda Hejazi et al, The Astronomical Journal 170 1

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The continuation of Figure 2 for the analyzed T...

The continuation of Figure 2 for the analyzed Ti I and Fe I lines.

Neda Hejazi et al, The Astronomical Journal 170 1

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Comparison between the observed spectrum (red d...

Comparison between the observed spectrum (red dots) and the best-fit model (blue lines) ...

Neda Hejazi et al, The Astronomical Journal 170 1

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The continuation of Figures 2 and 3 for the ana...

The continuation of Figures 2 and 3 for the analyzed V I lines. The line data used in th...

Neda Hejazi et al, The Astronomical Journal 170 1

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The continuum-normalized synthetic spectra asso...

The continuum-normalized synthetic spectra associated with the star’s parameters but wit...

Neda Hejazi et al, The Astronomical Journal 170 1

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The continuum-normalized synthetic spectra asso...

The continuum-normalized synthetic spectra associated with the star’s parameters but wit...

Neda Hejazi et al, The Astronomical Journal 170 1

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A small portion of the γ R2 0-0 TiO band used i...

A small portion of the γ R2 0-0 TiO band used in measuring the oxygen abundance. Top: co...

Neda Hejazi et al, The Astronomical Journal 170 1

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Identical to Figure 7, but for two analyzed Ti ...

Identical to Figure 7, but for two analyzed Ti I lines.

Neda Hejazi et al, The Astronomical Journal 170 1

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Identical to Figure 7, but for one analyzed Fe ...

Identical to Figure 7, but for one analyzed Fe I line.

Neda Hejazi et al, The Astronomical Journal 170 1

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Model lightcurves for typical novae (left) and ...

Model lightcurves for typical novae (left) and the specific Nova Vulpeculae 1968 after J...

Boshun Yang et al, The Astronomical Journal 170 1

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Search field of the 1408 (super)nova. The verti...

Search field of the 1408 (super)nova. The vertical dashed lines represent the boundaries...

Boshun Yang et al, The Astronomical Journal 170 1

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Observation drawn by M. Hevelius (1670; left) a...

Observation drawn by M. Hevelius (1670; left) and lightcurve (right) of the Nova Vul 167...

Boshun Yang et al, The Astronomical Journal 170 1

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Near-IR color–magnitude and color–color diagram...

Near-IR color–magnitude and color–color diagrams for adopted members of Upper Sco (Table...

K. L. Luhman, The Astronomical Journal 170 1

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Near-IR spectra of brown dwarf candidates in Up...

Near-IR spectra of brown dwarf candidates in Upper Sco. The Gemini data have been binned...

K. L. Luhman, The Astronomical Journal 170 1

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Near-IR spectra of brown dwarf candidates in Up...

Near-IR spectra of brown dwarf candidates in Upper Sco. The Gemini data have been binned...

K. L. Luhman, The Astronomical Journal 170 1

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Near-IR color–magnitude diagram for members of ...

Near-IR color–magnitude diagram for members of Upper Sco that have spectral classificati...

K. L. Luhman, The Astronomical Journal 170 1

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Proper motion offsets vs. parallactic distance ...

Proper motion offsets vs. parallactic distance based on Gaia DR3 for members of Upper Sc...

K. L. Luhman, The Astronomical Journal 170 1

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Mass vs. spectral type for young stars with mea...

Mass vs. spectral type for young stars with measurements of dynamical masses (Section 5....

K. L. Luhman, The Astronomical Journal 170 1

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IMFs for Upper Sco, Taurus, IC 348, Chamaeleon ...

IMFs for Upper Sco, Taurus, IC 348, Chamaeleon I, and the solar neighborhood. The normal...

K. L. Luhman, The Astronomical Journal 170 1

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W1−W2 vs. spectral type for late-type members o...

W1−W2 vs. spectral type for late-type members of Upper Sco. At

K. L. Luhman, The Astronomical Journal 170 1

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Analysis of filter outputs z∗ and ζ∗ from full ...

Analysis of filter outputs z∗ and ζ∗ from full solar system integrations using the same ...

Richard E. Zeebe and Ilja J. Kocken, The Astronomical Journal 170 1

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Illustration of synthetic filter outputs z∗ for...

Illustration of synthetic filter outputs z∗ for g3 and g4 (see Equation (12)) and associ...

Richard E. Zeebe and Ilja J. Kocken, The Astronomical Journal 170 1

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Differences in angles Δθ between a run with bot...

Differences in angles Δθ between a run with both J2 and mA increased, i.e., (J2, ×fmA) =...

Richard E. Zeebe and Ilja J. Kocken, The Astronomical Journal 170 1

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Analysis of g frequencies. (a) Moving-window FF...

Analysis of g frequencies. (a) Moving-window FFT power of Earth’s ﹩k=e\cos (\varpi )﹩ of...

Richard E. Zeebe and Ilja J. Kocken, The Astronomical Journal 170 1

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Analysis of s frequencies. (a) Moving-window FF...

Analysis of s frequencies. (a) Moving-window FFT power of Earth’s ...

Richard E. Zeebe and Ilja J. Kocken, The Astronomical Journal 170 1

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