JWST Reveals a Candidate Supermassive Black Hole Binary at z = 4.3 in the Brightest Submillimeter Galaxy in COSMOS-Web
Authors:
- Jed McKinneyJed McKinney
- Ansh GuptaAnsh Gupta
- Julian B. MuñozJulian B. Muñoz
- John ChisholmJohn Chisholm
- Caitlin M. CaseyCaitlin M. Casey
- Stephanie M. Urbano StawinskiStephanie M. Urbano Stawinski
- Olivia CooperOCOlivia Cooper
- Erini LambridesELErini Lambrides
- Hollis AkinsHollis Akins
- Maximilien FrancoMaximilien Franco
- Archana AravindanArchana Aravindan
- Seiji FujimotoSeiji Fujimoto
Open Access
- 30 October 2026
- journal article
- Published by American Astronomical Society in The Astrophysical Journal Letters
- Vol. 1011 (1) , L35
Abstract
We present JWST/NIRSpec PRISM and G395M grating spectroscopy for AzTEC-1, a massive submillimeter bright galaxy at z = 4.34 in the COSMOS extragalactic field. The PRISM spectrum reveals strong H α , a significant Balmer break, and no H β detection, indicating a 100–400 Myr old stellar population and high dust attenuation. Baldwin–Phillips–Terlevich (BPT) line ratios indicate the presence of an active galactic nucleus (AGN). Decomposing narrow- and broad-line components, we recover broad, blueshifted H α with a velocity offset of 1245 km s −1 from the systemic narrow-line velocity and with FWHM ≈ 2500 km s −1 . AzTEC-1’s smooth morphology and stellar age is suggestive of a past merger-induced starburst period that would have brought in a second supermassive black hole (SMBH), raising the possibility for a binary SMBH system. In this scenario, we assume that the lower-mass black hole (BH) hosts a broad-line region orbiting a quiescent primary. Evidence for an extended outflow is not found in the 2D spectrum, NIRCam imaging, resolved Atacama Large Millimeter/submillimeter Array (ALMA) observations of dust continuum, or CO, [C ii ] 157 μ m , and [N ii ] 2 05 μ m kinematics. AzTEC-1’s high central gas-mass surface density and dynamically unstable gas disk indicate that massive gas clouds external to the candidate binary SMBH’s orbit might have played a role in stalling infall from O ( 10 Myr) to O ( 100 Myr) through dynamical torques, which has been theorized to occur in the nuclei of massive galaxies like AzTEC-1. If the SMBH binary is confirmed, AzTEC-1 would be an excellent laboratory into the astrophysics driving low-frequency gravitational-wave detections.Keywords
Funding Information
- Space Telescope Science Institute (NAS5-26555)
- NSF ∣ National Science Foundation Graduate Research Fellowship Program (DGE 2137420)
- National Science Foundation (2503202)
- National Science Foundation (AST-2307354)
- National Science Foundation (AST-2408637)
- National Science Foundation (AST-2408247)
- Space Telescope Science Institute (HST-GO-16686)
- Space Telescope Science Institute (HST-AR-17028)
- Space Telescope Science Institute (JWST-GO-03788)
- Space Telescope Science Institute (JWST-AR-06278)
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