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Median 1.8 m spectra of PS, constructed by taki...

Median 1.8 m spectra of PS, constructed by taking the pixel-by-pixel median of individua...

T. J. Davidge, The Astronomical Journal 169 1

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Spectra recorded with the 1.8 m telescope on th...

Spectra recorded with the 1.8 m telescope on the night of 1939 March 4. The hour angle a...

T. J. Davidge, The Astronomical Journal 169 1

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Composite 1975 campaign spectrum of PS, constru...

Composite 1975 campaign spectrum of PS, constructed from the five spectra recorded durin...

T. J. Davidge, The Astronomical Journal 169 1

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Selected spectra in the wavelength interval 430...

Selected spectra in the wavelength interval 4300–4500 Å that were recorded during the 19...

T. J. Davidge, The Astronomical Journal 169 1

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Mean 1922 campaign spectra in the orbital phase...

Mean 1922 campaign spectra in the orbital phase intervals 0.15–0.35 and 0.65–0.85. The h...

T. J. Davidge, The Astronomical Journal 169 1

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Same as Figure 6, but comparing the 1937 campai...

Same as Figure 6, but comparing the 1937 campaign spectra. As in Figure 6, (1) the spect...

T. J. Davidge, The Astronomical Journal 169 1

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Same as Figure 4, but showing Hβ. Hβ is on the ...

Same as Figure 4, but showing Hβ. Hβ is on the shoulder of the response curve where the ...

T. J. Davidge, The Astronomical Journal 169 1

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Same as Figure 6, but comparing the 1975 campai...

Same as Figure 6, but comparing the 1975 campaign spectra. The wavelength interval cover...

T. J. Davidge, The Astronomical Journal 169 1

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Comparing line profiles near phases 0.25 and 0....

Comparing line profiles near phases 0.25 and 0.75. The black lines are the mean profiles...

T. J. Davidge, The Astronomical Journal 169 1

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Comparisons with synthetic spectra. The spectra...

Comparisons with synthetic spectra. The spectra of PS are the means of many of the 1.8 m...

T. J. Davidge, The Astronomical Journal 169 1

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Comparing campaign and synthetic spectra. The s...

Comparing campaign and synthetic spectra. The spectra of PS are the means of the 1.8 m s...

T. J. Davidge, The Astronomical Journal 169 1

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Spectra from the 1922 campaign that sample orbi...

Spectra from the 1922 campaign that sample orbital phases near 0.25 and 0.75 are compare...

T. J. Davidge, The Astronomical Journal 169 1

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CCFs of 1.8 m spectra near orbital phases 0.25 ...

CCFs of 1.8 m spectra near orbital phases 0.25 and 0.75 from the 1922 (top row) and 1937...

T. J. Davidge, The Astronomical Journal 169 1

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Same as Figure 13, but showing CCFs constructed...

Same as Figure 13, but showing CCFs constructed from 1.2 m spectra. The peak due to the ...

T. J. Davidge, The Astronomical Journal 169 1

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Radial velocities measured from digitized 1.8 m...

Radial velocities measured from digitized 1.8 m spectra using different techniques. The ...

T. J. Davidge, The Astronomical Journal 169 1

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Distributions of M*/L ratios at the W1 (a) and ...

Distributions of M*/L ratios at the W1 (a) and IRAC1 (b) bands. The gray-shaded histogra...

Taehyun Kim et al, The Astronomical Journal 169 1

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Dependence of M*/L calculated using the total l...

Dependence of M*/L calculated using the total luminosity on the W1−W2 color (a) and IRAC...

Taehyun Kim et al, The Astronomical Journal 169 1

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M*/L ratios calculated using the total luminosi...

M*/L ratios calculated using the total luminosity (a) and their scatters (b) as function...

Taehyun Kim et al, The Astronomical Journal 169 1

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Distributions of stellar and dust masses derive...

Distributions of stellar and dust masses derived from the SED fitting of multiwavelength...

Taehyun Kim et al, The Astronomical Journal 169 1

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Distributions of stellar masses and SFRs derive...

Distributions of stellar masses and SFRs derived from the SED fitting of multiwavelength...

Taehyun Kim et al, The Astronomical Journal 169 1

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M*/L calculated using the stellar luminosity (a...

M*/L calculated using the stellar luminosity (a) and their scatters (b) as functions of ...

Taehyun Kim et al, The Astronomical Journal 169 1

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W1−W2 color as a function of the ratio of the d...

W1−W2 color as a function of the ratio of the dust flux to the total flux at the W1 band...

Taehyun Kim et al, The Astronomical Journal 169 1

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Correlation between the flux ratio the dust at ...

Correlation between the flux ratio the dust at 3 μm (fdust,3 μm) and the color index bet...

Taehyun Kim et al, The Astronomical Journal 169 1

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Correlation between M*/L and stellar mass (M*) ...

Correlation between M*/L and stellar mass (M*) at ∼1.6 μm. Note that M*/L is calculated ...

Taehyun Kim et al, The Astronomical Journal 169 1

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Scatter in M*/L after correcting the correlatio...

Scatter in M*/L after correcting the correlation between M*/L and the stellar mass (M*)....

Taehyun Kim et al, The Astronomical Journal 169 1

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