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Comparison of cosmic-ray scattering rates in wa...

Comparison of cosmic-ray scattering rates in warm ionized medium predicted by YL08 and v...

Huirong Yan et al, The Astrophysical Journal Letters 1006 2

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(a) Collisionless damping rate of fast modes ve...

(a) Collisionless damping rate of fast modes versus the wavenumbers k⊥ and k∥ normalized...

Huirong Yan et al, The Astrophysical Journal Letters 1006 2

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Comparisons of (a) Dμμ and (b) scattering rate ...

Comparisons of (a) Dμμ and (b) scattering rate ν = Dμμ/(1 − μ2) between theoretical calc...

Huirong Yan et al, The Astrophysical Journal Letters 1006 2

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(a) Contour map of rms fractional deviation of ...

(a) Contour map of rms fractional deviation of the fitting between the theoretical and e...

Huirong Yan et al, The Astrophysical Journal Letters 1006 2

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Results of The Joker and the joint fitting of R...

Results of The Joker and the joint fitting of RV and astrometry. Panel (a): Keplerian or...

Yinghao Xu et al, The Astrophysical Journal Letters 1006 2

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SED fitting of G6096 from joint SED and dynamic...

SED fitting of G6096 from joint SED and dynamical results. The black line shows the best...

Yinghao Xu et al, The Astrophysical Journal Letters 1006 2

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Test results for the ﹩v{\rm{\sin }}i﹩ measureme...

Test results for the ﹩v{\rm{\sin }}i﹩ measurement. The red dashed line shows the ...

Yinghao Xu et al, The Astrophysical Journal Letters 1006 2

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Position of G6096 on the HR diagram. The backgr...

Position of G6096 on the HR diagram. The background stars are plotted for comparison, wh...

Yinghao Xu et al, The Astrophysical Journal Letters 1006 2

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Spectral disentangling results for q = 0.92 (=...

Spectral disentangling results for q = 0.92 (=1.14/1.24) at phases of large redshift an...

Yinghao Xu et al, The Astrophysical Journal Letters 1006 2

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Comparison of the observed spectrum of G6096 wi...

Comparison of the observed spectrum of G6096 with the best-fit template. The black line ...

Yinghao Xu et al, The Astrophysical Journal Letters 1006 2

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Comparison of inner (Pin) and outer (Pout) orbi...

Comparison of inner (Pin) and outer (Pout) orbital periods for triple systems from D. R....

Yinghao Xu et al, The Astrophysical Journal Letters 1006 2

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Relation between luminosity and color for a (se...

Relation between luminosity and color for a (semiresolved) stellar population with varyi...

Ignacio Martín-Navarro et al, The Astrophysical Journal Letters 1006 2

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(Top) The I-band brightness profile is shown in...

(Top) The I-band brightness profile is shown in blue, with the regions corresponding to ...

Ignacio Martín-Navarro et al, The Astrophysical Journal Letters 1006 2

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Individual fit. The corner plot represents the ...

Individual fit. The corner plot represents the posterior distribution for one representa...

Ignacio Martín-Navarro et al, The Astrophysical Journal Letters 1006 2

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Stellar population–based distance to the Androm...

Stellar population–based distance to the Andromeda galaxy. Light-gray lines correspond t...

Ignacio Martín-Navarro et al, The Astrophysical Journal Letters 1006 2

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The best-fitting age (left), metallicity (middl...

The best-fitting age (left), metallicity (middle), and Mr (right) measurements for 100 t...

Ignacio Martín-Navarro et al, The Astrophysical Journal Letters 1006 2

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Posterior coverage plot for the age (blue line)...

Posterior coverage plot for the age (blue line), metallicity (green line), and Mr (red l...

Ignacio Martín-Navarro et al, The Astrophysical Journal Letters 1006 2

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An output plot from the ATSAT pipeline depictin...

An output plot from the ATSAT pipeline depicting two plots of a signal that was flagged ...

Chenoa D. Tremblay et al, The Astrophysical Journal Letters 1006 2

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Geometry of the LTT 3780 planetary system at th...

Geometry of the LTT 3780 planetary system at the time of our radio technosignature obser...

Chenoa D. Tremblay et al, The Astrophysical Journal Letters 1006 2

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The event from Figure 2 centered to 2400.014593...

The event from Figure 2 centered to 2400.014593 MHz (bottom row) shown below two prior f...

Chenoa D. Tremblay et al, The Astrophysical Journal Letters 1006 2

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Weighted sky map of our sample, smoothed with a...

Weighted sky map of our sample, smoothed with a Gaussian filter (σ = 5). The image is sc...

Xianhao Ye et al, The Astrophysical Journal Letters 1006 2

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Proposed member candidates selected for the NGC...

Proposed member candidates selected for the NGC 5024 stream. Left panel: stream member c...

Xianhao Ye et al, The Astrophysical Journal Letters 1006 2

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Simulated tidal streams of NGC 5024 and Gaia CM...

Simulated tidal streams of NGC 5024 and Gaia CMD. Left panel: NGC 5024 and its mock stre...

Xianhao Ye et al, The Astrophysical Journal Letters 1006 2

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Our member candidates compared with simulated m...

Our member candidates compared with simulated member stars of NGC 5024 (red) and NGC 505...

Xianhao Ye et al, The Astrophysical Journal Letters 1006 2

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The [Fe/H]–RV plane and proper motion distribut...

The [Fe/H]–RV plane and proper motion distributions for the GCs NGC 5024 and NGC 5053, a...

Xianhao Ye et al, The Astrophysical Journal Letters 1006 2

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