Latest Images
Left: the canvas (approximately 14,000 × 13,000...
Top: distribution of the signal-to-noise ratio ...
Top: histogram of the mean apparent magnitude o...
From left to right, stacked cutouts of 2003 BF9...
Cutouts of each of the recovered sources. Objec...
Trajectory of 2003 BF91 on the sky as seen by H...
Here we plot the systemic velocity of CV Ser bo...
Finson–Probstein model overlays for C/2023 A3 (...
VLTI/GRAVITY interferometric data (colored) and...
Architecture of planetary orbits after the tida...
Similar to Figure 1 in the main text, but with ...
Similar to Figure 2 in the main text, but with ...
Parameter space in the ap − eb,0 plane showing ...
Evolution of a stellar binary (black) with four...
The evolution of nine-planet system during tida...
Same system as in Figure 1, but with mutual gra...
Similar to Figure 1, but including mutual gravi...
Apparent F1500W (left) and F1000W (right) magni...
White dwarf physical properties. (Top) Fit of t...
ePSF fitting indicates that MEAD 62 B is an un...
Left: inferred mass for the candidate companion...
Color composite of the MEAD 62 MIRI field with ...
Distributions of per-line zero-point offsets Δl...
Bootstrap test using Fe I VALD combined curves ...
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