Speaker
Franz Bauer
(Universidad Católica de Chile)
Description
Over the past few decades, multi-wavelength surveys have revolutionized our understanding of active galactic nuclei (AGN) demography, structure, physics, host galaxies and host/AGN co-evolution. Wide-field and deep X-rays and mid-infrared constraints have been particularly essential in this regard as a means to peer through the substantial dust obscuration that surrounds most strongly accreting supermassive black holes, while radio emission has provided a pivotal window for probing relativistic jets. With this review, I aim to highlight some of the key discoveries and advancements that have led us to our current understanding and outlook for the future.
Primary author
Franz Bauer
(Universidad Católica de Chile)
