SED Fitting

The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z∼2.3$
We present a study of spatially-resolved star formation histories for 60 z~2.3 main-sequence, star-forming galaxies. The results suggest that selecting star-forming galaxies at cosmic noon frequently includes systems in an “evolved” evolutionary phase where the centers have recently started a burst of star formation activity that will likely initiate inside-out quenching in the next several hundred million years.
Sam E. Cutler, Mauro Giavalisco, Zhiyuan Ji, Yingjie Cheng
PDF Cite Project DOI ADS
The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z∼2.3$
Resolved SED fitting with Prospector
Star formation histories of the inner and outer components of main sequence galaxies using resolved SED fitting
Resolved SED fitting with Prospector