Astronomy Image Explorer

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Top left: raw image including overscan/bias str...

Top left: raw image including overscan/bias strips. Top center: overscan removed, synthe...

Mike Alexandersen et al, The Planetary Science Journal 7 8

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Same as the upper left, lower left, and lower r...

Same as the upper left, lower left, and lower right panels of Figure 1, but zoomed in on...

Mike Alexandersen et al, The Planetary Science Journal 7 8

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Same as bottom right panel of Figure 2, but wit...

Same as bottom right panel of Figure 2, but with different donut parameters. Top row: ho...

Mike Alexandersen et al, The Planetary Science Journal 7 8

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Single image detection efficiency as a function...

Single image detection efficiency as a function of magnitude (left) and rate of motion (...

Mike Alexandersen et al, The Planetary Science Journal 7 8

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Single image detection efficiency as a function...

Single image detection efficiency as a function of rate, using h = 40 (left), h = 100 (m...

Mike Alexandersen et al, The Planetary Science Journal 7 8

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Multi-image detection efficiency as a function ...

Multi-image detection efficiency as a function of magnitude (left) and rate of motion (r...

Mike Alexandersen et al, The Planetary Science Journal 7 8

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“Shift+stack” images, showing 49′ × 49′ cutouts...

“Shift+stack” images, showing 49′ × 49′ cutouts centered on the dwarf planet (90377) Sed...

Mike Alexandersen et al, The Planetary Science Journal 7 8

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Images cleaned using donut template subtraction...

Images cleaned using donut template subtraction with hole size h = 40 and dough width d ...

Mike Alexandersen et al, The Planetary Science Journal 7 8

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Sketch for the RS Oph ejecta inferred from SED ...

Sketch for the RS Oph ejecta inferred from SED models (side view, Section 4.1). Due to t...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Examples of the observed (in magenta) and model...

Examples of the observed (in magenta) and modeled (black lines) SEDs of RS Oph at select...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Evolution of the Hα line parameters. Left: the ...

Evolution of the Hα line parameters. Left: the broad component is shown. The flux (panel...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Examples of SED models in the UV/optical/near-I...

Examples of SED models in the UV/optical/near-IR domain. Given the similarity of the RS ...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Example of the evolution of the broad and narro...

Example of the evolution of the broad and narrow components of the hydrogen line profile...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Mass-loss rate by the ionized part of the eject...

Mass-loss rate by the ionized part of the ejecta, ﹩{\dot{M}}_{{\rm{WD}}}﹩ (panel (a)) an...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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The B, V, and IC LCs (panel (a)), and evolution...

The B, V, and IC LCs (panel (a)), and evolution in LWD (b), ...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Comparison of V and visual LCs of RS Oph around...

Comparison of V and visual LCs of RS Oph around the maxima of its explosions in 2021, 20...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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The ratio of fluxes from the warm WDP, ...

The ratio of fluxes from the warm WDP, ﹩{F}_{{\rm{WD}}}^{{\rm{warm}}}﹩, and the nebula, ...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Comparison of the warm WDP luminosity (...

Comparison of the warm WDP luminosity (﹩{L}_{{\rm{WD}}}^{{\rm{warm}}}﹩, Table 3), the lu...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Evolution of the continuum fluxes, Fcont., at/a...

Evolution of the continuum fluxes, Fcont., at/around selected emission lines (see keys) ...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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The evolution of the RS Oph optical spectrum me...

The evolution of the RS Oph optical spectrum measured by the UVES spectrograph from day ...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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Evolution of the Hα (left) and Hβ (right) line ...

Evolution of the Hα (left) and Hβ (right) line profiles during the first hours and days ...

Augustin Skopal et al, The Astrophysical Journal 1007 2

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E-mode and B-mode power spectra, CEE and CBB, c...

E-mode and B-mode power spectra, CEE and CBB, calculated from synthetic dust polarizatio...

Yue Hu et al, The Astrophysical Journal 1007 2

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(a–c) Distributions of the relative angle θρ, θ...

(a–c) Distributions of the relative angle θρ, θv, and θB between the local magnetic fiel...

Yue Hu et al, The Astrophysical Journal 1007 2

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Statistical properties of scale-dependent veloc...

Statistical properties of scale-dependent velocity and magnetic field fluctuations decom...

Yue Hu et al, The Astrophysical Journal 1007 2

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Ratio of CEE to CBB from synthetic dust polariz...

Ratio of CEE to CBB from synthetic dust polarization at 353 GHz. Top panel: EE and BB po...

Yue Hu et al, The Astrophysical Journal 1007 2

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