The AGN–Star Formation Connection: Future Prospects with JWST

The AGN–Star Formation Connection: Future Prospects with JWST

The bulk of the stellar growth over cosmic time is dominated by IR-luminous galaxies at cosmic noon (z = 1-2), many of which harbor a hidden active galactic nucleus (AGN). We use state-of-the-art infrared color diagnostics, combining Spitzer and Herschel observations, to separate dust-obscured AGNs...

Full description

Bibliographic Details
Main Authors: Kirkpatrick, Allison, Alberts, Stacey, Pope, Alexandra, Barro, Guillermo, Bonato, Matteo, Kocevski, Dale D., Pérez-González, Pablo, Rieke, George H., Rodríguez-Muñoz, Lucia, Sajina, Anna, Grogin, Norman A., Mantha, Kameswara Bharadwaj, Pandya, Viraj, Pforr, Janine, Salvato, Mara, Santini, Paola
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
galaxies: active
galaxies: photometry
galaxies: star formation
Online Access:http://hdl.handle.net/10150/626176
http://arizona.openrepository.com/arizona/handle/10150/626176

Internet

http://hdl.handle.net/10150/626176
http://arizona.openrepository.com/arizona/handle/10150/626176

Similar Items