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The top panel shows the along-scan residuals (m...

The top panel shows the along-scan residuals (mas) of the fit of Gaia FPR data set, bott...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Photocenter offset as function of the solar pha...

Photocenter offset as function of the solar phase angle for objects of 0.1, 1 and 10 km ...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Orbital fit residuals of asteroid 779 Nina (H =...

Orbital fit residuals of asteroid 779 Nina (H = 8.02) using the photocenter correction (...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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The top panel shows the length of the observati...

The top panel shows the length of the observation arc as function of the absolute magnit...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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The asteroid position relative to the observer ...

The asteroid position relative to the observer ρ ...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Uncertainty in the semimajor axis of the 20,536...

Uncertainty in the semimajor axis of the 20,536 asteroids with H < 14 and σ ...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Transit weighted mean of along-scan residuals (...

Transit weighted mean of along-scan residuals (mas) from Gaia FPR data set. The orange b...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Normalized along-scan residuals (mas) with resp...

Normalized along-scan residuals (mas) with respect to the uncertainty in the measurement...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Uncertainty in the semimajor axis normalized by...

Uncertainty in the semimajor axis normalized by the semimajor axis. We include the uncer...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Normalized orbital fit residuals of asteroid 35...

Normalized orbital fit residuals of asteroid 3557 Sokolsky (H = 11.06), using the photoc...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Semimajor axis prediction test: truncating the ...

Semimajor axis prediction test: truncating the observational arc until 2017 June 1 (subs...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Semimajor axis prediction tests of the 20,915 a...

Semimajor axis prediction tests of the 20,915 asteroids with H < 14 and σ ...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Semimajor axis difference between long-arc solu...

Semimajor axis difference between long-arc solutions of the 20,915 asteroids with H < 14...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Sensitivity of the semimajor axis to perturber ...

Sensitivity of the semimajor axis to perturber masses via Monte Carlo as a function of t...

Oscar Fuentes-Muñoz et al, The Astronomical Journal 167 6

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Sample spectra showing the features of HF at 23...

Sample spectra showing the features of HF at 23359 Å and Na I at 23379 Å used in this an...

K. E. Brady et al, The Astronomical Journal 167 6

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The observed and synthetic spectra for the (1−0...

The observed and synthetic spectra for the (1−0) R9 2.3358 μm feature of the HF molecule...

K. E. Brady et al, The Astronomical Journal 167 6

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Derived abundance vs. effective temperature, wi...

Derived abundance vs. effective temperature, with metallicity ([Fe/H]) indicated by color.

K. E. Brady et al, The Astronomical Journal 167 6

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[F/Fe] (upper panel) and [Na/Fe] (lower panel) ...

[F/Fe] (upper panel) and [Na/Fe] (lower panel) vs. [Fe/H] for thick disk (red circles), ...

K. E. Brady et al, The Astronomical Journal 167 6

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[F/Fe] vs. [Fe/H] for our sample of thin- and t...

[F/Fe] vs. [Fe/H] for our sample of thin- and thick-disk stars with measurements from th...

K. E. Brady et al, The Astronomical Journal 167 6

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[F/O] vs. [O/H] for our sample of thin- and thi...

[F/O] vs. [O/H] for our sample of thin- and thick-disk stars with measurements from the ...

K. E. Brady et al, The Astronomical Journal 167 6

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Comparison between our best fit and recent high...

Comparison between our best fit and recent high-redshift observations of the MZR made by...

Andrew Marszewski et al, The Astrophysical Journal Letters 967 2

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The gas-phase MZR in our simulations at z = 8 c...

The gas-phase MZR in our simulations at z = 8 calculated using different weighting schem...

Andrew Marszewski et al, The Astrophysical Journal Letters 967 2

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The gas fractions, f gas =...

The gas fractions, f gas = M gas/M ...

Andrew Marszewski et al, The Astrophysical Journal Letters 967 2

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The evolution of the gas-phase MZR in FIRE-2 si...

The evolution of the gas-phase MZR in FIRE-2 simulations from z = 5 to 12. The solid bla...

Andrew Marszewski et al, The Astrophysical Journal Letters 967 2

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Comparison between the MZR at z = 5 from the hi...

Comparison between the MZR at z = 5 from the high-redshift suite of FIRE-2 simulations a...

Andrew Marszewski et al, The Astrophysical Journal Letters 967 2

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