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Data, Quasar point source model, quasar-subtrac...

Data, Quasar point source model, quasar-subtracted, S/N, and smoothed S/N cubes of J0910...

Raymond P. Remigio et al, The Astrophysical Journal Letters 1003 1

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Left panel: the total flux (gray), extended Lyα...

Left panel: the total flux (gray), extended Lyα (red), and 1σ error (blue) extracted ove...

Raymond P. Remigio et al, The Astrophysical Journal Letters 1003 1

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Radial surface brightness profile of the extend...

Radial surface brightness profile of the extended emission (blue points). The radial bin...

Raymond P. Remigio et al, The Astrophysical Journal Letters 1003 1

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Moment maps of the extended Lyα around J0910−04...

Moment maps of the extended Lyα around J0910−0414. The leftmost image was created by app...

Raymond P. Remigio et al, The Astrophysical Journal Letters 1003 1

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Top panel: total flux spectrum (black) and the ...

Top panel: total flux spectrum (black) and the 1σ error spectrum (blue) extracted from t...

Raymond P. Remigio et al, The Astrophysical Journal Letters 1003 1

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X-ray lightcurves and spectra of the canonical ...

X-ray lightcurves and spectra of the canonical (Lc) model. Left panel: the X-ray lightcu...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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The time-resolved spectra in different models a...

The time-resolved spectra in different models and for different viewing angles. The soli...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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The Eiso versus Epeak diagram. The blue solid l...

The Eiso versus Epeak diagram. The blue solid line represents the Amati relation for the...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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The T90-averaged spectra in different models. C...

The T90-averaged spectra in different models. Colors represent different models, as in F...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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EP WXT (0.5–4 keV) lightcurves in different mod...

EP WXT (0.5–4 keV) lightcurves in different models. The blue, red, green, and purple lin...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Lightcurves at observer’s wavelength λ = 200 nm...

Lightcurves at observer’s wavelength λ = 200 nm (≈NUV band). Colors represent different ...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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The temporal evolutions of the peak energy in d...

The temporal evolutions of the peak energy in different models. Colors represent differe...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Late-time bolometric lightcurves (left axis) fo...

Late-time bolometric lightcurves (left axis) for different models viewed at θv = 45°. Co...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Time-resolved spectra at late times. The solid ...

Time-resolved spectra at late times. The solid lines are spectra at 0.1 days, and the da...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Energy density maps, the sum of the kinetic ene...

Energy density maps, the sum of the kinetic energy density ...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Upper panel: bolometric lightcurves (including ...

Upper panel: bolometric lightcurves (including all bands, i.e., X-ray/UV/optical) for th...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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The angular distributions of the isotropic-equi...

The angular distributions of the isotropic-equivalent energy Eiso (solid lines, left axi...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Optical lightcurves at λ = 555 nm (≈V band). So...

Optical lightcurves at λ = 555 nm (≈V band). Solid lines (θv = 10°) and dashed lines (θv...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Nonthermal X-ray “prompt emission” at Eobs = 1 ...

Nonthermal X-ray “prompt emission” at Eobs = 1 keV in the observer’s frame, based on the...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Left panel: the energy distribution per logarit...

Left panel: the energy distribution per logarithm of the terminal four-velocity. The blu...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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The ratio η (Equation (B1)) between energy dens...

The ratio η (Equation (B1)) between energy density and free–free energy production. The ...

Jian-He Zheng and Wenbin Lu, The Astrophysical Journal Letters 1003 1

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Energy dependence of the 10 s accumulated elect...

Energy dependence of the 10 s accumulated electron precipitation fraction ...

Feiyu Yu et al, The Astrophysical Journal Letters 1003 1

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3D magnetic configuration and current sheet at ...

3D magnetic configuration and current sheet at 03:52 UT in the MHD model. (a) Distributi...

Feiyu Yu et al, The Astrophysical Journal Letters 1003 1

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Temporal evolution of precipitating electron co...

Temporal evolution of precipitating electron counts at different energies under four tur...

Feiyu Yu et al, The Astrophysical Journal Letters 1003 1

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Distribution of 10 s accumulated precipitating ...

Distribution of 10 s accumulated precipitating electrons mapped to the magnetogram at th...

Feiyu Yu et al, The Astrophysical Journal Letters 1003 1

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