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Two examples of the initial orbit locations in ...

Dynamical Modeling of Galaxies and Supe...

Two examples of the initial orbit locations in the x–z start space. Two nearly axisymmet...

The Astrophysical Journal Supplement Series 254 2 25

(Top panel) Relationship between the viewing an...

Dynamical Modeling of Galaxies and Supe...

(Top panel) Relationship between the viewing angle ψ and the triaxiality of the deprojec...

The Astrophysical Journal Supplement Series 254 2 25

Illustration of the issue with setting the zero...

Dynamical Modeling of Galaxies and Supe...

Illustration of the issue with setting the zero-point of the logarithmic potential to Φ0...

The Astrophysical Journal Supplement Series 254 2 25

Illustration of the changing MBH constraints in...

Dynamical Modeling of Galaxies and Supe...

Illustration of the changing MBH constraints in NGC 1453 as the orbit model goes through...

The Astrophysical Journal Supplement Series 254 2 25

The same as the left panel of Figure 4 but show...

Dynamical Modeling of Galaxies and Supe...

The same as the left panel of Figure 4 but showing the azimuthal dependence of the origi...

The Astrophysical Journal Supplement Series 254 2 25

The same as Figure 1 but for two additional mas...

Dynamical Modeling of Galaxies and Supe...

The same as Figure 1 but for two additional mass models with larger triaxiality: (left) ...

The Astrophysical Journal Supplement Series 254 2 25

Illustration of the MBH constraints for the moc...

Dynamical Modeling of Galaxies and Supe...

Illustration of the MBH constraints for the mock data sets described in the text. Each d...

The Astrophysical Journal Supplement Series 254 2 25

Lowest 10 adiabatic eigenvalue curves for the c...

Lyman and Balmer Continuum Spectra for ...

Lowest 10 adiabatic eigenvalue curves for the continuum state ﹩{m}^{{\pi }_{z}}={1}^{-}﹩...

The Astrophysical Journal Supplement Series 254 2 21

Balmer continuum spectra, calculated with the a...

Lyman and Balmer Continuum Spectra for ...

Balmer continuum spectra, calculated with the adiabatic-basis-expansion method, for phot...

The Astrophysical Journal Supplement Series 254 2 21

Same as Figure 2, but for the 2s0 → 1+ photoion...

Lyman and Balmer Continuum Spectra for ...

Same as Figure 2, but for the 2s0 → 1+ photoionization process.

The Astrophysical Journal Supplement Series 254 2 21

Same as Figure 2, but for the 2p0 → 0+ photoion...

Lyman and Balmer Continuum Spectra for ...

Same as Figure 2, but for the 2p0 → 0+ photoionization process.

The Astrophysical Journal Supplement Series 254 2 21

Same as Figure 2, but for the 2p0 → ( − 1)− pho...

Lyman and Balmer Continuum Spectra for ...

Same as Figure 2, but for the 2p0 → ( − 1)− photoionization process.

The Astrophysical Journal Supplement Series 254 2 21

Same as Figure 2, but for the 2p−1 → 0+ photoio...

Lyman and Balmer Continuum Spectra for ...

Same as Figure 2, but for the 2p−1 → 0+ photoionization process.

The Astrophysical Journal Supplement Series 254 2 21

Same as Figure 2, but for the 2p−1 → ( − 2)+ ph...

Lyman and Balmer Continuum Spectra for ...

Same as Figure 2, but for the 2p−1 → ( − 2)+ photoionization process.

The Astrophysical Journal Supplement Series 254 2 21

Comparison of Balmer continuum spectra for the ...

Lyman and Balmer Continuum Spectra for ...

Comparison of Balmer continuum spectra for the photoionization processes (a) 2p−1 → 0+ a...

The Astrophysical Journal Supplement Series 254 2 21

Comparison of Balmer continuum spectra for the ...

Lyman and Balmer Continuum Spectra for ...

Comparison of Balmer continuum spectra for the photoionization processes at γ = 0.05 au ...

The Astrophysical Journal Supplement Series 254 2 21

Lyman continuum spectra, calculated with the co...

Lyman and Balmer Continuum Spectra for ...

Lyman continuum spectra, calculated with the coupled-channel theory (Zhao et al. 2016), ...

The Astrophysical Journal Supplement Series 254 2 21

Same as Figure 10, but Balmer continuum spectra...

Lyman and Balmer Continuum Spectra for ...

Same as Figure 10, but Balmer continuum spectra for the 2s0 → 0− photoionization process.

The Astrophysical Journal Supplement Series 254 2 21

Same as Figure 10, but Balmer continuum spectra...

Lyman and Balmer Continuum Spectra for ...

Same as Figure 10, but Balmer continuum spectra for the 2s0 → 1+ photoionization process.

The Astrophysical Journal Supplement Series 254 2 21

Same as Figure 10, but Balmer continuum spectra...

Lyman and Balmer Continuum Spectra for ...

Same as Figure 10, but Balmer continuum spectra for the 2p0 → 1− photoionization process.

The Astrophysical Journal Supplement Series 254 2 21

Comparison of Lyman and Balmer continuum spectr...

Lyman and Balmer Continuum Spectra for ...

Comparison of Lyman and Balmer continuum spectra for the photoionization processes (a) 1...

The Astrophysical Journal Supplement Series 254 2 21

The Y3 DES core data sets and their relationshi...

Dark Energy Survey Year 3 Results: Phot...

The Y3 DES core data sets and their relationships. Arrows indicate information flow from...

The Astrophysical Journal Supplement Series 254 2 24

The DES footprint in equatorial coordinates, in...

Dark Energy Survey Year 3 Results: Phot...

The DES footprint in equatorial coordinates, including the Wide Survey, the Supernova Su...

The Astrophysical Journal Supplement Series 254 2 24

Left: area covered to a certain magnitude limit...

Dark Energy Survey Year 3 Results: Phot...

Left: area covered to a certain magnitude limit in 2″ diameter apertures for each data r...

The Astrophysical Journal Supplement Series 254 2 24

Astrometric residuals of Y3 GOLD vs. Gaia’s DR2...

Dark Energy Survey Year 3 Results: Phot...

Astrometric residuals of Y3 GOLD vs. Gaia’s DR2 objects, computed as the median value of...

The Astrophysical Journal Supplement Series 254 2 24

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