Latest Images
System architectures and HZ boundaries for the ...
Percentage of the simulation that the injected ...
The mass and semimajor axis of a possible lost ...
The eccentricity distribution of giant planets ...
Angular separation of Gaia-4b (solid line) and ...
A central binary will remove some material, red...
Top: dust mass as a function of projected dista...
Membership diagnostics among the sources in our...
Disk dust mass distribution for the tight binar...
Infrared color–color diagrams using photometry ...
HCO+ detections, including moment 0 maps (in un...
Continuum images, centered on the detections, o...
Continuum images, centered on the detections, o...
Location of our tight binary targets on a map o...
The fields observed by the UKIRT team during th...
Map of the ﹩{A}_{{K}_{S}}﹩ extinction of the Re...
Shown are two example fields of stars that pass...
﹩{2}^{{\prime} }\times {2}^{{\prime} }﹩ map of...
K-band filter used by the UKIRT microlensing su...
Mapping of the exponential gradient parameter, ...
Illumination corrections for the 2017 UKIRT mic...
Fit results for two sample fields of standard, ...
Comparison of extinction maps from this work wi...
Comparison of ﹩{A}_{{K}_{S}}/E(H-{K}_{S})﹩ from...
ANNOUNCEMENTS
Take the AstroExplorer for a spin!
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!
