Uncovering the First AGN Jets with AXIS

Author:

Connor Thomas1ORCID,Bañados Eduardo2ORCID,Cappelluti Nico3ORCID,Foord Adi4ORCID

Affiliation:

1. Center for Astrophysics | Harvard & Smithsonian, 60 Garden St., Cambridge, MA 02138, USA

2. Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany

3. Department of Physics, University of Miami, Coral Gables, FL 33124, USA

4. Department of Physics, University of Maryland Baltimore County, 1000 Hilltop Cir, Baltimore, MD 21250, USA

Abstract

Jets powered by AGN in the early Universe (z≳6) have the potential to not only define the evolutionary trajectories of the first-forming massive galaxies but to enable the accelerated growth of their associated SMBHs. Under typical assumptions, jets could even rectify observed quasars with light seed formation scenarios; however, not only are constraints on the parameters of the first jets lacking, observations of these objects are scarce. Owing to the significant energy density of the CMB at these epochs capable of quenching radio emission, observations will require powerful, high angular resolution X-ray imaging to map and characterize these jets. As such, AXIS will be necessary to understand early SMBH growth and feedback. This White Paper is part of a series commissioned for the AXIS Probe Concept Mission; additional AXIS White Papers can be found at the AXIS website.

Publisher

MDPI AG

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