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Redshift evolution of rest-frame J-band galaxy ...

Redshift evolution of rest-frame J-band galaxy effective radius (Re,J; left) and dust-ex...

Si-Yue Yu et al, The Astrophysical Journal Letters 1005 1

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Redshift evolution of intrinsic rest-frame J-ba...

Redshift evolution of intrinsic rest-frame J-band surface brightness, μJ, corrected for ...

Si-Yue Yu et al, The Astrophysical Journal Letters 1005 1

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Rest-frame color–color diagram for our galaxy s...

Rest-frame color–color diagram for our galaxy sample in three redshift bins. The individ...

Si-Yue Yu et al, The Astrophysical Journal Letters 1005 1

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Comparison of the best-fit size evolution at a ...

Comparison of the best-fit size evolution at a fixed stellar mass of M⋆ = 5 × 1010M⊙ bet...

Si-Yue Yu et al, The Astrophysical Journal Letters 1005 1

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Average dependence of Re on rest-frame waveleng...

Average dependence of Re on rest-frame wavelength for SFGs (left) and QGs (right) at 1 <...

Si-Yue Yu et al, The Astrophysical Journal Letters 1005 1

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We simulate the rise, peak, and initial decay o...

We simulate the rise, peak, and initial decay of a TDE using MCRT + 1D hydrodynamics. To...

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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The blue, green, and orange lines show the outp...

The blue, green, and orange lines show the output SED using three different opacity pres...

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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This cartoon depicts the main components of a w...

This cartoon depicts the main components of a wind-reprocessed TDE. In our simulation, w...

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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Top: we find that adiabatic losses result in a ...

Top: we find that adiabatic losses result in a peak luminosity that is ∼6× lower than t...

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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Top: fraction of oxygen in different ionization...

Top: fraction of oxygen in different ionization states as a function of radius at two re...

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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We compare 3 epochs of our simulation with Sedo...

We compare 3 epochs of our simulation with Sedona non-LTE postprocessing results from L....

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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Relevant hydro quantities as a function of time...

Relevant hydro quantities as a function of time and radius from the fiducial simulation ...

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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Here, we compare the SED evolution for simulati...

Here, we compare the SED evolution for simulations with three different values of the li...

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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The advected pulse problem solved analytically ...

The advected pulse problem solved analytically in the diffusion approximation (solid lin...

Brenna Mockler et al, The Astrophysical Journal Letters 1005 1

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Estimated ACF (normalized) ...

Estimated ACF (normalized) ﹩{\hat{R}}_{b}(\ell )={\hat{C}}_{b}(\ell )/{\hat{C}}_{b}(0)﹩ ...

Jean C. Perez et al, The Astrophysical Journal Letters 1005 1

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Left panels: comparison of biased vs. unbiased ...

Left panels: comparison of biased vs. unbiased ACF estimates for T = 6 hr (top) and T = ...

Jean C. Perez et al, The Astrophysical Journal Letters 1005 1

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Top left: the estimated PSD at zero frequency f...

Top left: the estimated PSD at zero frequency for each of the four ACF estimates, and th...

Jean C. Perez et al, The Astrophysical Journal Letters 1005 1

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Top: normalized local-mean-variance (left axis)...

Top: normalized local-mean-variance (left axis), ...

Jean C. Perez et al, The Astrophysical Journal Letters 1005 1

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﹩{C}_{h,N}^{(+)}(\ell )﹩ (forward) and ...

﹩{C}_{h,N}^{(+)}(\ell )﹩ (forward) and ﹩{C}_{h,N}^{(-)}(\ell )﹩ (backward) ACF estimati...

Jean C. Perez et al, The Astrophysical Journal Letters 1005 1

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Observations of TOI-1710 A. (a) NEID RVs, after...

Observations of TOI-1710 A. (a) NEID RVs, after subtracting a long-term linear trend (pu...

Juan I. Espinoza-Retamal et al, The Astrophysical Journal Letters 1005 1

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Results of the ensemble of secular simulations....

Results of the ensemble of secular simulations. The semimajor axis of the intermediate c...

Juan I. Espinoza-Retamal et al, The Astrophysical Journal Letters 1005 1

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Secular evolution of the obliquities of TOI-171...

Secular evolution of the obliquities of TOI-1710 from four-body secular integrations. Th...

Juan I. Espinoza-Retamal et al, The Astrophysical Journal Letters 1005 1

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Mass–semimajor axis diagram for the hypothetica...

Mass–semimajor axis diagram for the hypothetical intermediate companion. The points are ...

Juan I. Espinoza-Retamal et al, The Astrophysical Journal Letters 1005 1

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The half-mass radius rh• (blue), core radius rc...

The half-mass radius rh• (blue), core radius rc• (red), average mass ...

Yining Sun and Long Wang, The Astrophysical Journal Letters 1005 1

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Density profiles as a function of radius for M5...

Density profiles as a function of radius for M50k-IMF-BH and M50k-IMF-ALL under differen...

Yining Sun and Long Wang, The Astrophysical Journal Letters 1005 1

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