Latest Images
Our sample of 17 massive quiescent galaxies is ...
The stellar mass vs. sSFR (in log scale, top pa...
Two-component pysersic fits for the galaxies in...
Nonparametric morphological parameters for our ...
Two-component pysersic fits for the galaxies in...
Top: this is an RGB image (using F444W, F356W, ...
Figures (a), (e), and (i) are the RGB images (u...
Mean radial profiles for the stellar mass, SFR,...
Mean radial profiles of the U − V and V − J col...
Mean radial profiles of the formation time (t50...
SFHs for all galaxies in our sample from BAGPIP...
Morphological parameters as a function of redsh...
BAGPIPES posterior corner plots for the three l...
The H I sensitivity limits across surveys. Scat...
The H I versus stellar mass distribution of the...
Summary of the nearby H I–bearing host galaxies...
The H I mass (MH I) versus velocity line width ...
The spatial and kinematic separations between t...
The number of dwarf satellites within the host’...
Atomic gas fraction (...
The number of H I–bearing satellite candidates ...
Satellite gas depletion versus host halo mass, ...
Satellite–host spatial (dproj) and velocity (ΔV...
Key ingredients of our injection method for ass...
ANNOUNCEMENTS
We have updated the search and sort algorithm to return records in reverse chronological order based on the date/time that the images were uploaded to the Astronomy Image Explorer. This is potentially but rarely different from the publication date. Thank you!