Uncovering the First AGN Jets with AXIS

dc.contributor.authorConnor, Thomas
dc.contributor.authorBañados, Eduardo
dc.contributor.authorCappelluti, Nico
dc.contributor.authorFoord, Adi
dc.date.accessioned2023-12-04T15:15:25Z
dc.date.available2023-12-04T15:15:25Z
dc.date.issued2023-11-14
dc.description.abstractJets powered by AGN in the early Universe (z ≳ 6) have the potential to not only define the 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.
dc.description.urihttps://arxiv.org/abs/2311.08451
dc.format.extent7 pages
dc.genrejournal articles
dc.genrepreprints
dc.genrewhite papers
dc.identifier.urihttps://doi.org/10.48550/arXiv.2311.08451
dc.identifier.urihttp://hdl.handle.net/11603/31007
dc.language.isoen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Physics Department Collection
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.titleUncovering the First AGN Jets with AXIS
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0002-1616-1701

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