Latest Images
Left panels: comparison between spectroscopical...
Comparison between spectroscopically inferred v...
Our best-fit effective temperatures for young (...
Best-fit sedimentation efficiency fsed derived ...
Stacked spectral residuals of our young (<300 M...
Cumulative distributions (solid lines) of the b...
Stacked spectral residuals of our young (<300 M...
Cumulative distributions (solid lines) of the b...
The observed (black) and best-fit model spectra...
χ2-based spectral fitting results of three repr...
Comparison of spectroscopically inferred Teff, ...
J-band absolute magnitudes and J − K colors of ...
Ages and bolometric luminosities of our benchma...
Spectral type distribution of our sample of ben...
Best-fit synthetic spectra for all targets usin...
Best-fit synthetic spectra for all targets usin...
Absolute difference in BIC between spectral fit...
Best-fit extinction coefficient from spectral f...
Comparison of parameters derived from the Sonor...
R.A. and decl. residuals for the GRAVITY observ...
Predicted separation of both β Pic b and c in o...
Relationship between the K-band brightness rati...
Upper mass limits for a potential lunar compani...
Formation of external magnetic enhancements abo...
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Be sure to try the search and sorting features, which were added based on user feedback; browse and find the links to videos and interactive figures in our Journal articles; find AAS Research Notes; or notice that new publishers have begun adding their figures to the AIE. Get in touch to hear more!