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(Top) Model uncertainties for the fluorescence ...

(Top) Model uncertainties for the fluorescence spectrum of Ni I, calculated as the stand...

S. J. Bromley et al, The Planetary Science Journal 7 5

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From top to bottom: (1) Ni I synthetic spectrum...

From top to bottom: (1) Ni I synthetic spectrum (red) at the orbital conditions of Hyaku...

S. J. Bromley et al, The Planetary Science Journal 7 5

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Fluorescence spectra stick plots on a logarithm...

Fluorescence spectra stick plots on a logarithmic intensity scale with the strongest lin...

S. J. Bromley et al, The Planetary Science Journal 7 5

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Comparison of Ni I (left) and Fe I fluorescence...

Comparison of Ni I (left) and Fe I fluorescence models (in photon units) to the observed...

S. J. Bromley et al, The Planetary Science Journal 7 5

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Ratio of fluorescence efficiency standard devia...

Ratio of fluorescence efficiency standard deviation to fluorescence efficiency (in perce...

S. J. Bromley et al, The Planetary Science Journal 7 5

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Comparison of fluorescence efficiencies (with g...

Comparison of fluorescence efficiencies (with geometric factors) and observed fluxes of ...

S. J. Bromley et al, The Planetary Science Journal 7 5

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(# bins = 10) of [Ni/OH], [Fe/OH], [Ni/CN], [Fe...

(# bins = 10) of [Ni/OH], [Fe/OH], [Ni/CN], [Fe/CN], and [Ni/Fe] in log10 for all comets...

S. J. Bromley et al, The Planetary Science Journal 7 5

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Sensitivity of our modeled fluorescence efficie...

Sensitivity of our modeled fluorescence efficiencies for some representative Ni I lines ...

S. J. Bromley et al, The Planetary Science Journal 7 5

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Calculated fluorescence efficiencies for observ...

Calculated fluorescence efficiencies for observed metal lines in Hyakutake as a function...

S. J. Bromley et al, The Planetary Science Journal 7 5

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Top: model uncertainties for the fluorescence s...

Top: model uncertainties for the fluorescence spectrum of Ni I, calculated as the standa...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Synthetic fluorescence spectra stick plots on a...

Synthetic fluorescence spectra stick plots on a logarithmic intensity scale with the str...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Ratio of line intensity standard deviation to l...

Ratio of line intensity standard deviation to line intensity (in percentage) for 213 Ni ...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Top: spatial distributions of nickel, iron, and...

Top: spatial distributions of nickel, iron, and molecular lines normalized to 1 at photo...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Sensitivity of our modeled fluorescence efficie...

Sensitivity of our modeled fluorescence efficiencies for some representative Ni I lines ...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Histograms (# bins = 10) of [Ni/OH], [Fe/OH], [...

Histograms (# bins = 10) of [Ni/OH], [Fe/OH], [Ni/CN], [Fe/CN], and [Ni/Fe] in log10 for...

S. J. Bromley et al, The Planetary Science Journal 2 6

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From top to bottom: (1) Ni I synthetic spectrum...

From top to bottom: (1) Ni I synthetic spectrum (red) at the orbital conditions of Hyaku...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Comparison of Ni I (left) and Fe I (right) line...

Comparison of Ni I (left) and Fe I (right) line intensities of our fluorescence model to...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Comparison of modeled and observed line intensi...

Comparison of modeled and observed line intensities of Ni I (left) and Fe I (right). Mod...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Grotrian diagrams of Ni I (top) and Fe I (botto...

Grotrian diagrams of Ni I (top) and Fe I (bottom) showing the observed emission lines of...

S. J. Bromley et al, The Planetary Science Journal 2 6

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Calculated fluorescence efficiencies for observ...

Calculated fluorescence efficiencies for observed metal lines in Hyakutake as a function...

S. J. Bromley et al, The Planetary Science Journal 2 6

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The left panel shows the timing results for the...

The left panel shows the timing results for the glitch at MJD 54904. Panels (a) and (b) ...

Wen-Tao Ye et al, The Astrophysical Journal Letters 1003 2

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Pulse peak separation and amplitude ratio measu...

Pulse peak separation and amplitude ratio measured in 60 day intervals. Panel (a) shows ...

Wen-Tao Ye et al, The Astrophysical Journal Letters 1003 2

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The flux of the two pulse peaks. The diamond an...

The flux of the two pulse peaks. The diamond and square points represent the flux of P1 ...

Wen-Tao Ye et al, The Astrophysical Journal Letters 1003 2

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Simultaneous ASKAP radio and TESS optical obser...

Simultaneous ASKAP radio and TESS optical observations of ASKAP J181335−604720. Top pane...

Shouzhi Wang et al, The Astrophysical Journal Letters 1003 2

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TESS photometric analysis of ASKAP J181335−6047...

TESS photometric analysis of ASKAP J181335−604720 (TIC 365466012). (a) Sector 93 TESS PD...

Shouzhi Wang et al, The Astrophysical Journal Letters 1003 2

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