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The two panels show Δχ2 as a function of parent...

The two panels show Δχ2 as a function of parent scale length (Lp) of HCN for November 5 ...

Timothy N. Proudkii et al, The Planetary Science Journal 7 5

(A) HCN (J = 3–2) spectrum of A1 on UT 2021 Nov...

(A) HCN (J = 3–2) spectrum of A1 on UT 2021 November 5 (black). The top panel shows the ...

Timothy N. Proudkii et al, The Planetary Science Journal 7 5

Evolution of the CS (NOEMA: J = 5–4; APEX: J = ...

Evolution of the CS (NOEMA: J = 5–4; APEX: J = 7–6, 5–4) spectral line in comet A1. The ...

Timothy N. Proudkii et al, The Planetary Science Journal 7 5

Spectrally integrated flux maps for HCN (J = 3–...

Spectrally integrated flux maps for HCN (J = 3–2) detections on November 5 (left) and No...

Timothy N. Proudkii et al, The Planetary Science Journal 7 5

Evolution of the HCN (NOEMA: J = 3–2; APEX: J =...

Evolution of the HCN (NOEMA: J = 3–2; APEX: J = 4–3) spectral line in comet A1. The blac...

Timothy N. Proudkii et al, The Planetary Science Journal 7 5

Preperihelion time evolution (decreasing rH) of...

Preperihelion time evolution (decreasing rH) of the CS (top) and HCN (bottom) mixing rat...

Timothy N. Proudkii et al, The Planetary Science Journal 7 5

Preperihelion time evolution (decreasing rH) of...

Preperihelion time evolution (decreasing rH) of the CS/HCN mixing ratio in comet A1. Bec...

Timothy N. Proudkii et al, The Planetary Science Journal 7 5

Spacecraft trajectory to Torifune from Earth de...

Spacecraft trajectory to Torifune from Earth departure in 2020 December to the flyby in ...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 5

Hayabusa2# mission spaceflight operation scenario.

Hayabusa2# mission spaceflight operation scenario.

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 5

Variations in the solar phase angle (spacecraft...

Variations in the solar phase angle (spacecraft–asteroid–Sun angle) and the spacecraft–a...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 5

Tentative planning for flyby science observatio...

Tentative planning for flyby science observation sequences. “Sat. search” means satellit...

Masatoshi Hirabayashi et al, The Planetary Science Journal 7 5

Left: the orbital parameter space of the WD-MBH...

Left: the orbital parameter space of the WD-MBH system in which diffusive-tide rpTDEs ar...

Shu Yan Lau et al, The Astrophysical Journal Letters 1003 2

Left: parameter-space plot showing the evolutio...

Left: parameter-space plot showing the evolution of the MS-MBH binary (α = 0.8) for diff...

Shu Yan Lau et al, The Astrophysical Journal Letters 1003 2

Left: evolution of the f-mode energy for a WD a...

Left: evolution of the f-mode energy for a WD and two MS models with α = 0.3 and 0.8, or...

Shu Yan Lau et al, The Astrophysical Journal Letters 1003 2

Left: time between successive mass-ejection epi...

Left: time between successive mass-ejection episodes as a function of episode number occ...

Shu Yan Lau et al, The Astrophysical Journal Letters 1003 2

As in Figure 4, but with a binary SNR threshold...

As in Figure 4, but with a binary SNR threshold of 8, yielding fzlk = 5.0 (thermal) and ...

Wen-Fan Feng et al, The Astrophysical Journal Letters 1003 2

Dual-line gravitational radiation excitation th...

Dual-line gravitational radiation excitation through the ZLK effect for the Galactic Cen...

Wen-Fan Feng et al, The Astrophysical Journal Letters 1003 2

SNR contours for continuous GW detection from r...

SNR contours for continuous GW detection from rapidly spinning NSs at the Galactic Cente...

Wen-Fan Feng et al, The Astrophysical Journal Letters 1003 2

Geometric configuration of the hierarchical tri...

Geometric configuration of the hierarchical triple system where an NS binary orbits Sgr ...

Wen-Fan Feng et al, The Astrophysical Journal Letters 1003 2

As in the right panel of Figure 3, but for unif...

As in the right panel of Figure 3, but for uniform eccentricity sampling, yielding fzlk ...

Wen-Fan Feng et al, The Astrophysical Journal Letters 1003 2

Spatial distributions of three most distant sta...

Spatial distributions of three most distant star-forming regions with precise distance m...

Xianjin Shen et al, The Astronomical Journal 171 6

Parallax fitting results without incorporating ...

Parallax fitting results without incorporating geodetic blocks. The top panels present t...

Xianjin Shen et al, The Astronomical Journal 171 6

12CO(J = 1–0) spectrum of the star-forming regi...

12CO(J = 1–0) spectrum of the star-forming region G040.96+02.48. The spectral profile is...

Xianjin Shen et al, The Astronomical Journal 171 6

Distance PDFs for star-forming region G040.96+0...

Distance PDFs for star-forming region G040.96+02.48. The term “kinematic” denotes the PD...

Xianjin Shen et al, The Astronomical Journal 171 6

Same as Figure 1 but with consideration of geod...

Same as Figure 1 but with consideration of geodetic blocks.

Xianjin Shen et al, The Astronomical Journal 171 6

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