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Median values of the O/H (left; ...

Median values of the O/H (left; ﹩{\mathrm{log}}_{10}﹩ parts per trillion) and C/O (right...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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O/H (top) and C/H (bottom) in ...

O/H (top) and C/H (bottom) in ﹩{\mathrm{log}}_{10}﹩ parts per trillion as a function of ...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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Measured atmospheric abundances in WASP-178b fr...

Measured atmospheric abundances in WASP-178b from J. D. Lothringer et al. (2025a; transp...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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C/O ratio as a function of metallicity [M/H] as...

C/O ratio as a function of metallicity [M/H] as given in Table 4. Planets observed with ...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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Measured atmospheric abundances in WASP-17b fro...

Measured atmospheric abundances in WASP-17b from D. R. Louie et al. (2025; black points ...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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Metallicity as a function of equilibrium temper...

Metallicity as a function of equilibrium temperature for planets in the eclipse (magenta...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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Top: mass–metallicity trend parameter constrain...

Top: mass–metallicity trend parameter constraints using Equation (5) for the different o...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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C/O ratio as a function of equilibrium temperat...

C/O ratio as a function of equilibrium temperature for planets in the eclipse (magenta s...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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C/O ratio vs. planet mass for our sample. Plane...

C/O ratio vs. planet mass for our sample. Planets observed with direct spectroscopy are ...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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Planet metallicity (top; as given in Table 4) a...

Planet metallicity (top; as given in Table 4) and C/O (bottom) vs. stellar mass (left) a...

Joshua D. Lothringer et al, The Astronomical Journal 171 1

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Top left panel: map of the Lupus targets analyz...

Top left panel: map of the Lupus targets analyzed in this work, with the IRIS 100 μm map...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Comparison between imag and idisk,gas. The dash...

Comparison between imag and idisk,gas. The dashed line indicates equality, and the shade...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Top panel: same as the top left panel of Figure...

Top panel: same as the top left panel of Figure 1, but with CTTS names labeled. Arrows a...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Consensus matrix for the 3D groups found from 5...

Consensus matrix for the 3D groups found from 5000 MC iterations of HDBSCAN, using min_c...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Same as Figure 4, but for the 4D groups. Roman ...

Same as Figure 4, but for the 4D groups. Roman numerals indicate the assigned groups, an...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Clustering procedure tests, where points are co...

Clustering procedure tests, where points are colored by cluster assignment. Filled point...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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New flow model fits to VLT Hα profiles from X-S...

New flow model fits to VLT Hα profiles from X-Shooter (XS), UVES, and ESPRESSO (ESP). Co...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Inclination uniformity test. Top: ...

Inclination uniformity test. Top: ﹩\cos ({i}_{{\rm{mag}}})﹩ histogram (left) and CDF (ri...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Hα profile dependence on imag for 6 CTTSs in ou...

Hα profile dependence on imag for 6 CTTSs in our sample, with all other accretion flow m...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Maps of the Orion (top left), Taurus (top right...

Maps of the Orion (top left), Taurus (top right), and Chamaeleon I (bottom) targets from...

Caeley V. Pittman et al, The Astrophysical Journal Letters 994 2

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Integrated flux map of the 12CO (J = 2–1) emis...

Integrated flux map of the 12CO (J = 2–1) emission around Sgr A*. The map is primary be...

Mark D. Gorski and Lena Murchikova, The Astrophysical Journal Letters 995 2

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The full map of the CND in ...

The full map of the CND in ﹩\mathrm{HCN}(J=1\mbox{--}0)﹩ emission from P.-Y. Hsieh et al...

Mark D. Gorski and Lena Murchikova, The Astrophysical Journal Letters 995 2

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Left: comoving formation rate ρ(z) of FXTs obta...

Left: comoving formation rate ρ(z) of FXTs obtained from Equation (6). It is normalized ...

Yizhou Guo et al, The Astrophysical Journal Letters 995 2

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Left: cumulative luminosity function ψ(L0,X). T...

Left: cumulative luminosity function ψ(L0,X). The scatter represents the cumulative numb...

Yizhou Guo et al, The Astrophysical Journal Letters 995 2

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The X-ray luminosity versus redshift of 31 FXTs...

The X-ray luminosity versus redshift of 31 FXTs. The solid (black) curve shows the trunc...

Yizhou Guo et al, The Astrophysical Journal Letters 995 2

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