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Top panels: The amplitude of bulk flow in the r...

Top panels: The amplitude of bulk flow in the redshifts 0.1 < z < 0.2. Middle panels: Th...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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Top panels: The direction of bulk flow in the r...

Top panels: The direction of bulk flow in the redshifts 0.1 < z < 0.2. Middle panels: Th...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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Top panel: The bulk flow direction pointing tow...

Top panel: The bulk flow direction pointing toward (l, b) = (330° ± 15°, −16° ± 17°) in ...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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Top panel: The bulk flow direction pointing tow...

Top panel: The bulk flow direction pointing toward (l, b) = (255° ±22°, 59° ± 28°) in th...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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Comparison of different models on the CMB power...

Comparison of different models on the CMB power spectrum.

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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Top panel: The bulk flow direction pointing tow...

Top panel: The bulk flow direction pointing toward (l, b) = (332° ±18°, 69° ± 18°) in th...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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Top panels: The direction of bulk flow in the r...

Top panels: The direction of bulk flow in the redshifts 0.001 < z < 0.016. Middle panels...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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Top panels: The amplitude of bulk flow in the r...

Top panels: The amplitude of bulk flow in the redshifts 0.001 < z < 0.016. Middle panels...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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The bulk flow direction pointing toward (l, b) ...

The bulk flow direction pointing toward (l, b) = (306 ± 16, −12 ± 14) in the redshift 0....

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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The bulk flow direction pointing toward (l, b) ...

The bulk flow direction pointing toward (l, b) = (122° ± 20°, −25° ± 18°) in the redshif...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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The bulk flow direction pointing toward (l, b) ...

The bulk flow direction pointing toward (l, b) = (305° ± 25°, 23° ± 20°) in the redshift...

Muhammad Yarahmadi and Amin Salehi, The Astronomical Journal 169 3

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Green lines present the predicted shadow path's...

Green lines present the predicted shadow path's northern and southern limits, with the 1...

F. L. Rommel et al, The Planetary Science Journal 6 2

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Objects’ densities as a function of diameter. T...

Objects’ densities as a function of diameter. The square marks the location of Huya usin...

F. L. Rommel et al, The Planetary Science Journal 6 2

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Occultation light curves of the Huya system as ...

Occultation light curves of the Huya system as recorded on (a) 2021 March 28, (b) 2023 F...

F. L. Rommel et al, The Planetary Science Journal 6 2

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Stellar occultation by Huya on 2023 June 24 wit...

Stellar occultation by Huya on 2023 June 24 with the location of the stations that had i...

F. L. Rommel et al, The Planetary Science Journal 6 2

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Stellar occultations by the Huya system observe...

Stellar occultations by the Huya system observed on (a) 2021 March 28, (b) 2023 February...

F. L. Rommel et al, The Planetary Science Journal 6 2

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A comparison of the Keplerian orbit solution an...

A comparison of the Keplerian orbit solution and the observational data. The black ellip...

F. L. Rommel et al, The Planetary Science Journal 6 2

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Ring radial width as a function of ring apparen...

Ring radial width as a function of ring apparent opacity (﹩p^{\prime} ﹩), considering th...

F. L. Rommel et al, The Planetary Science Journal 6 2

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Target star flux ratio (red) with uncertainties...

Target star flux ratio (red) with uncertainties (gray) as a function of time for the thr...

F. L. Rommel et al, The Planetary Science Journal 6 2

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Huya’s limb as observed during the stellar occu...

Huya’s limb as observed during the stellar occultation in 2019 March 28 (P. Santos-Sanz ...

F. L. Rommel et al, The Planetary Science Journal 6 2

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A corner plot of the MCMC chains from the satel...

A corner plot of the MCMC chains from the satellite orbit fit. The two-dimensional conto...

F. L. Rommel et al, The Planetary Science Journal 6 2

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(a) H3+ emission from Io’s auroral footprint (n...

(a) H3+ emission from Io’s auroral footprint (north) as seen at limb, created using 32 L...

A. Mura et al, The Planetary Science Journal 6 2

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Seven observations (radiance maps in the L band...

Seven observations (radiance maps in the L band) of the south IFP taken during Juno’s or...

A. Mura et al, The Planetary Science Journal 6 2

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Temporal variability for the mean radiance with...

Temporal variability for the mean radiance within the ROI for (a) orbit 13 and (b) orbit...

A. Mura et al, The Planetary Science Journal 6 2

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Corner plot for the MCMC model (orbit 13 only)....

Corner plot for the MCMC model (orbit 13 only). The two diagonal elements show the 1D ma...

A. Mura et al, The Planetary Science Journal 6 2

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