Latest Images
Cartoon illustrating a plausible formation and ...
Top: JWST/NIRCam cutouts in three filters (F115...
Same as Figure 1, but showing residual images f...
RGB composites of the full LRD sample. All imag...
The total LW magnitude of the companion(s), MLW...
Left panel: effective projected separation betw...
RGB composite of the A68 cluster field, constru...
Left: panels (A) and (B) show the residual meri...
Time–latitude profile of variations in the resi...
Panel (A) shows the temporal and latitudinal ev...
First and last images from an example in our tr...
Receiver operating characteristic (ROC) curves ...
SMDET neural network architecture. The input (t...
Density of 176″ × 176″ sky regions that scored ...
Gallery of first and last images in SMDET input...
Validation loss during SMDET training (Section ...
Comparisons between SMDET (x-axes) and J. D. Ki...
Histograms comparing the number of fast (...
Effect of stellar metallicity control on the C/...
Comparison of stellar abundances between HARPS ...
Cross calibration of [C/H] and [O/H] between th...
Calibration of abundances from HARPS to KECK. T...
Calibration of abundances from SDSS to KECK. To...
Calibration of abundances from KECK to HARPS. T...
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