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Example SEDs of rebinned spaxels in the central...

Example SEDs of rebinned spaxels in the central regions of the four PHANGS-MUSE galaxies...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Contour plots showing the distribution of Spitz...

Contour plots showing the distribution of Spitzer/IRAC colors at 3.6 and 4.5 μm ([3.6] −...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Comparison of stellar kinematics between this s...

Comparison of stellar kinematics between this study and a previous PHANGS-MUSE study (E....

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Contour plots showing the distribution of outpu...

Contour plots showing the distribution of output parameters, including age, metallicity,...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Comparison of stellar population parameters bet...

Comparison of stellar population parameters between this study and a previous PHANGS-MUS...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Stellar mass-to-light ratios as a function of a...

Stellar mass-to-light ratios as a function of age, derived from the spectral templates f...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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SEDs in the wavelengths of 0.45−5.0 μm from SSP...

SEDs in the wavelengths of 0.45−5.0 μm from SSP templates, assuming a stellar age of ...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Example white light maps (left-hand column), re...

Example white light maps (left-hand column), resolved stellar mass maps (middle column),...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Dependence of the stellar mass-to-light ratio a...

Dependence of the stellar mass-to-light ratio at IRAC 3.6 μm on stellar age, derived usi...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Comparisons of stellar masses obtained from pPX...

Comparisons of stellar masses obtained from pPXF (x-axis) and values predicted by the be...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Comparisons of stellar masses obtained from pPX...

Comparisons of stellar masses obtained from pPXF (y-axis) with the values predicted by t...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Violin diagrams illustrating the distributions ...

Violin diagrams illustrating the distributions of mass-to-light ratios at IRAC 3.6 μm fo...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Scatter (standard deviation of the residuals in...

Scatter (standard deviation of the residuals in dex) of the best-fit linear model for th...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Logarithmic stellar mass differences between ou...

Logarithmic stellar mass differences between our pPXF results and the S4G survey, as a f...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Comparison of stellar masses from this study (p...

Comparison of stellar masses from this study (pPXF) with those derived from the WISE sca...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Comparisons of stellar masses obtained from the...

Comparisons of stellar masses obtained from the pPXF (x-axis) with the values predicted ...

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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Same as Figure A1, albeit for the difference in...

Same as Figure A1, albeit for the difference in luminosity at IRAC 3.6 μm.

Jeong Hwan Lee et al, The Astronomical Journal 169 3

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A comparison of a consistent and inconsistent t...

A comparison of a consistent and inconsistent treatment of microturbulent velocity. The ...

Ivan Hubeny et al, The Astronomical Journal 169 3

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Top two panels: model fit for eta UMa for the v...

Top two panels: model fit for eta UMa for the vturb = 2 km s–1 grid with the parameters ...

Ivan Hubeny et al, The Astronomical Journal 169 3

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A comparison in three wavelength regions of the...

A comparison in three wavelength regions of the current models (black) with the old Lanz...

Ivan Hubeny et al, The Astronomical Journal 169 3

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Gridpoints of the adopted model atmosphere grid...

Gridpoints of the adopted model atmosphere grids for which the spectra are calculated. B...

Ivan Hubeny et al, The Astronomical Journal 169 3

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A portion of UV spectrum for two fully consiste...

A portion of UV spectrum for two fully consistent models—one with vturb = 10 km s−1 (use...

Ivan Hubeny et al, The Astronomical Journal 169 3

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Continuum-subtracted MIRI-MRS spectra (reduced ...

Continuum-subtracted MIRI-MRS spectra (reduced by the JDISCS team; K. M. Pontoppidan et ...

Colette Salyk et al, The Astronomical Journal 169 3

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Upper-level energies of emission lines in the r...

Upper-level energies of emission lines in the regions highlighted in Section 4.2 (from t...

Colette Salyk et al, The Astronomical Journal 169 3

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Left: best-fit CO2 column density vs. temperatu...

Left: best-fit CO2 column density vs. temperature for published slab models. For 2MASS-J...

Colette Salyk et al, The Astronomical Journal 169 3

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