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Neutral densities, ionization rates, and ioniza...

Ionization Efficiency in the Dayside Ma...

Neutral densities, ionization rates, and ionization efficiencies for CO2 (blue) and O (r...

The Astrophysical Journal Letters 857 2 L18

Altitude profiles of CO2 (left) and O (right) i...

Ionization Efficiency in the Dayside Ma...

Altitude profiles of CO2 (left) and O (right) ionization efficiencies for the 240 nomina...

The Astrophysical Journal Letters 857 2 L18

Diurnal (top) and solar cycle (bottom) variatio...

Ionization Efficiency in the Dayside Ma...

Diurnal (top) and solar cycle (bottom) variations of CO2 (blue) and O (red) ionization e...

The Astrophysical Journal Letters 857 2 L18

Distribution of CO2 ionization efficiency at th...

Ionization Efficiency in the Dayside Ma...

Distribution of CO2 ionization efficiency at the top of the dayside Martian upper atmosp...

The Astrophysical Journal Letters 857 2 L18

Relative benefit Δ of an ideal search strategy ...

Optimal Target Stars in the Search for ...

Relative benefit Δ of an ideal search strategy as a function of stellar mass. The blue c...

The Astrophysical Journal Letters 857 2 L17

Relative benefit Δ for a direct-imaging search ...

Optimal Target Stars in the Search for ...

Relative benefit Δ for a direct-imaging search strategy as a function of stellar mass. T...

The Astrophysical Journal Letters 857 2 L17

Relative benefit Δ for a transmission spectrosc...

Optimal Target Stars in the Search for ...

Relative benefit Δ for a transmission spectroscopy search strategy as a function of stel...

The Astrophysical Journal Letters 857 2 L17

Left: XMM-Newton PN spectra for GSN 069  along...

A Long Decay of X-Ray Flux and Spectral...

Left: XMM-Newton PN spectra for GSN 069  along with the best-fitted models (top panel)....

The Astrophysical Journal Letters 857 2 L16

Upper panel: historical flux light curve in the...

A Long Decay of X-Ray Flux and Spectral...

Upper panel: historical flux light curve in the 0.2–2 keV for GSN 069. The Swift data a...

The Astrophysical Journal Letters 857 2 L16

Upper panel: the best-fitting χ2 values are plo...

A Long Decay of X-Ray Flux and Spectral...

Upper panel: the best-fitting χ2 values are plotted against the actual time of TDE from ...

The Astrophysical Journal Letters 857 2 L16

Upper panel: joint 68% (dotted) and 99% (solid)...

A Long Decay of X-Ray Flux and Spectral...

Upper panel: joint 68% (dotted) and 99% (solid) confidence contours of the blackbody tem...

The Astrophysical Journal Letters 857 2 L16

Power spectral densities of (red) the magnetic ...

von Kármán–Howarth Equation for Hall Ma...

Power spectral densities of (red) the magnetic field, (blue) the proton velocity field, ...

The Astrophysical Journal Letters 857 2 L19

Second-order structure functions of (red) the m...

von Kármán–Howarth Equation for Hall Ma...

Second-order structure functions of (red) the magnetic field, (blue) the proton velocity...

The Astrophysical Journal Letters 857 2 L19

Exact law in hybrid simulations βi = 1/16, βi =...

von Kármán–Howarth Equation for Hall Ma...

Exact law in hybrid simulations βi = 1/16, βi = 1/2, and βi = 4: The cascade rate, ϵ*, n...

The Astrophysical Journal Letters 857 2 L19

Orbit of the SMC around the LMC in the model wi...

Models of Tidally Induced Gas Filaments...

Orbit of the SMC around the LMC in the model with a 9:1 mass ratio. The orbit before ent...

The Astrophysical Journal 857 2 101

Tidal interaction between SMC and LMC before in...

Models of Tidally Induced Gas Filaments...

Tidal interaction between SMC and LMC before infall to the MW potential in the model wit...

The Astrophysical Journal 857 2 101

MS in gas according to our simulation with a 9:...

Models of Tidally Induced Gas Filaments...

MS in gas according to our simulation with a 9:1 LMC–SMC mass ratio. The top three panel...

The Astrophysical Journal 857 2 101

Dynamical age of the Stream in the model with a...

Models of Tidally Induced Gas Filaments...

Dynamical age of the Stream in the model with a 9:1 mass ratio color-coded by time since...

The Astrophysical Journal 857 2 101

MS in the stellar component according to our si...

Models of Tidally Induced Gas Filaments...

MS in the stellar component according to our simulation with a 9:1 LMC–SMC mass ratio. T...

The Astrophysical Journal 857 2 101

Line-of-sight velocity (in the frame of the loc...

Models of Tidally Induced Gas Filaments...

Line-of-sight velocity (in the frame of the local standard of rest) to the MS in the 9:1...

The Astrophysical Journal 857 2 101

Representation in Magellanic Stream coordinates...

Models of Tidally Induced Gas Filaments...

Representation in Magellanic Stream coordinates for interactions with different mass rat...

The Astrophysical Journal 857 2 101

Percentage of material stripped from both Cloud...

Models of Tidally Induced Gas Filaments...

Percentage of material stripped from both Clouds during their mutual interaction. The da...

The Astrophysical Journal 857 2 101

Intensity time profiles for the 41 “Hit” (corre...

A Short-term ESPERTA-based Forecast Too...

Intensity time profiles for the 41 “Hit” (correctly predicted) ≥S2 > 10 MeV proton event...

The Astrophysical Journal 857 2 107

ESPERTA probability contours for the prediction...

A Short-term ESPERTA-based Forecast Too...

ESPERTA probability contours for the prediction of ≥S1 SPEs for three solar longitude ba...

The Astrophysical Journal 857 2 107

ESPERTA probability contours for prediction of ...

A Short-term ESPERTA-based Forecast Too...

ESPERTA probability contours for prediction of ≥S2 SPEs for three solar longitude bands....

The Astrophysical Journal 857 2 107

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