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Representative SR model performance. Panel (a):...
Four main steps of our methodology. (1) Deep le...
Current helicity spatial distribution and chunk...
High correlations for MEAN and VAR terms, compu...
Schematic pictures of AGN+dense gas envelope mo...
Sample selection in this work. (a) We select LR...
Rest UV versus Hα line luminosity in LRDs (top)...
Lyα line equivalent widths of the sample broad ...
The effect of different size–luminosity relatio...
Histograms of the UV-to-Hα luminosity ratios fo...
NIRCam images of LRDs in this work. For each so...
Same as Figure 7 but for LBDs.
Dynamical evolution of a star–hot Jupiter syste...
Precession frequency evolution versus orbital p...
Stellar obliquity (ψ⋆) distributions sculpted b...
Evolution of fully retrograde systems (initial ...
Schematic of a hot Jupiter undergoing “lossy” R...
Similar to Figure 2, except with initial angula...
Schematic of population-level expectations for ...
“Lossy” Roche-lobe overflow of a hot Jupiter wi...
Post-Roche lobe overflow evolution of the plane...
Phase-folded light curve obtained with TESS of ...
Phase-folded RV curve of TOI-2040 b with the or...
Same as Figure 1 but for TOI-2578.
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