Latest Images

Residual maps and transmission spectra around H...

Residual maps and transmission spectra around Hα (left) and the He I NIR triplet (right)...

Tianjun Gan et al, The Astronomical Journal 171 2

The model of the RM and CLV (see Section 3.2) a...

The model of the RM and CLV (see Section 3.2) around the Na I doublet, normalized by the...

Tianjun Gan et al, The Astronomical Journal 171 2

Same as Figure 4 but for the Na I doublet lines...

Same as Figure 4 but for the Na I doublet lines (left panels) and K I λ7701 Å (right pan...

Tianjun Gan et al, The Astronomical Journal 171 2

Top panel: raw spectrum matrix around the Na I ...

Top panel: raw spectrum matrix around the Na I doublet. Middle panel: normalized spectru...

Tianjun Gan et al, The Astronomical Journal 171 2

The S/N of the spectra (red) near the Na I λλ58...

The S/N of the spectra (red) near the Na I λλ5891,5898 Å doublet lines and the airmass (...

Tianjun Gan et al, The Astronomical Journal 171 2

Same as Figure 4 but for the Ca II IRT lines: λ...

Same as Figure 4 but for the Ca II IRT lines: λ8500 Å (left), λ8544 Å (middle), λ8664 Å ...

Tianjun Gan et al, The Astronomical Journal 171 2

Cross-correlation results of HAT-P-70b with rob...

Cross-correlation results of HAT-P-70b with robust detections that have S/N ≥ 4 (top: Ca...

Tianjun Gan et al, The Astronomical Journal 171 2

Distribution of Hα observations for gas giants ...

Distribution of Hα observations for gas giants as a function of the stellar age vs. plan...

Tianjun Gan et al, The Astronomical Journal 171 2

Effective temperature vs. equilibrium temperatu...

Effective temperature vs. equilibrium temperature for the gas giant population (Rp ≳ 0.5...

Tianjun Gan et al, The Astronomical Journal 171 2

The cross-correlation results of VO using the t...

The cross-correlation results of VO using the template from B. Plez (top, P. Mollière et...

Tianjun Gan et al, The Astronomical Journal 171 2

The equilibrium temperature and planet radius d...

The equilibrium temperature and planet radius distribution of planets with either Fe I (...

Tianjun Gan et al, The Astronomical Journal 171 2

Same as Figure 7, but for the tentative detecti...

Same as Figure 7, but for the tentative detection of K I with 3 ≤ S/N < 4.

Tianjun Gan et al, The Astronomical Journal 171 2

The complete figure set (10 images) is availabl...

The complete figure set (10 images) is available in the online journal.

Tianjun Gan et al, The Astronomical Journal 171 2

The complete figure set (11 images) is availabl...

The complete figure set (11 images) is available in the online journal.

Tianjun Gan et al, The Astronomical Journal 171 2

Same as Figure 4 but for Li I λ6710 Å.

Same as Figure 4 but for Li I λ6710 Å.

Tianjun Gan et al, The Astronomical Journal 171 2

(a) Peak intensity image of the 217 GHz masers ...

(a) Peak intensity image of the 217 GHz masers surrounding MM1 at Epoch 2019.451, with s...

T. R. Hunter et al, The Astrophysical Journal Letters 997 1

Native-resolution peak intensity images of the ...

Native-resolution peak intensity images of the 217 GHz maser emission in grayscale, orde...

T. R. Hunter et al, The Astrophysical Journal Letters 997 1

(a) Light curve of the 199 and 217 GHz maser li...

(a) Light curve of the 199 and 217 GHz maser lines on a semilog scale overlaid by fitted...

T. R. Hunter et al, The Astrophysical Journal Letters 997 1

Power spectra of vortical motions obtained usin...

Power spectra of vortical motions obtained using modes in the range ℓ ∈ [70, 200] and 12...

Shravan M. Hanasoge, The Astrophysical Journal Letters 997 1

Power spectra of vortical motions obtained usin...

Power spectra of vortical motions obtained using modes in the range ℓ ∈ [70, 200] and 12...

Shravan M. Hanasoge, The Astrophysical Journal Letters 997 1

Vorticity spectra obtained using only f-modes i...

Vorticity spectra obtained using only f-modes in the range ℓ ∈ [200, 300] and 1293 ≤ ωnℓ...

Shravan M. Hanasoge, The Astrophysical Journal Letters 997 1

Rough estimates of the upper rupper (dashed red...

Rough estimates of the upper rupper (dashed red line) and lower rlow (solid blue line) t...

Shravan M. Hanasoge, The Astrophysical Journal Letters 997 1

Posterior distributions of the model parameters...

Posterior distributions of the model parameters from the MCMC fit. Diagonal panels show ...

Chunhua Qi et al, The Astrophysical Journal Letters 997 1

Two-dimensional posterior distribution of 16O/1...

Two-dimensional posterior distribution of 16O/18O versus ﹩\mathrm{log}{N}_{{\rm{CO}}}﹩ f...

Chunhua Qi et al, The Astrophysical Journal Letters 997 1

Radial profiles of the same-transition isotopol...

Radial profiles of the same-transition isotopologue intensity ratios. Left: C17O/13C18O(...

Chunhua Qi et al, The Astrophysical Journal Letters 997 1

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