Speaker
Description
We used a multiwavelength approach to study star-forming (SF) and active galactic nuclei (AGN)-dominated galaxies.
Unlike precedent works focused on individual wavelength regimes, we combined optical and infrared data, which we reprocessed using customized software in
order to enhance the data quality. This led to a better differentiation of the two main categories of galaxies that are indispensable to understanding galaxy
evolution (Yao et al. 2020). We incorporated early science continuum data from MeerKAT into our analysis (Yao et al. 2022).
Yao, H.~F.~M., Jarrett, T.~H., Cluver, M.~E., et al.\ 2020, \apj, 903, 91. doi:10.3847/1538-4357/abba1a
Yao, H.~F.~M., Cluver, M.~E., Jarrett, T.~H., et al.\ 2022, \apj, 939, 26. doi:10.3847/1538-4357/ac8790
| In-person or online? | in-person |
|---|---|
| keywords | cross-matching, source finding, imaging, AGN, star-forming galaxies |
| Career level | ECR |
