Searching for electromagnetic emission in an AGN from the gravitational wave binary black hole merger candidate S230922g

We carried out long-term monitoring of the LIGO/Virgo/KAGRA binary black hole (BBH) merger candidate S230922g in search of electromagnetic emission from the interaction of the merger remnant with an embedding active galactic nuclei (AGN) accretion disk. Using a dataset primarily composed of wide-field imaging from the Dark Energy Camera and supplemented by additional photometric and spectroscopic resources, we searched $\ensuremath{\sim}70%$ of the sky area probability for transient phenomena and discovered six counterpart candidates. One especially promising candidate---AT 2023aagj---exhibited temporally varying asymmetric components in spectral broad line regions, a feature potentially indicative of an off-center event such as a BBH merger. This represents the first live search and multiwavelength, photometric, and spectroscopic monitoring of a gravitational wave BBH optical counterpart candidate in the disk of an AGN.

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Journal
Physical review. D/Physical review. D.
Published
2024-12-20
DOI
https://doi.org/10.1103/physrevd.110.123029
Citations
15
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
4.97

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article

Searching for electromagnetic emission in an AGN from the gravitational wave binary black hole merger candidate S230922g

Barry McKernan, D. Gruen, K. E. Saavik Ford, A. Riffeser et al.
15 citations
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
4.97
article

Searching for electromagnetic emission in an AGN from the gravitational wave binary black hole merger candidate S230922g

Barry McKernan, D. Gruen, K. E. Saavik Ford, A. Riffeser, F. Valdés, M. J. Graham, A. Palmese, Brendan O’Connor, P. Clark, Julian S. Sommer, Tomás Cabrera, M. W. Coughlin, Igor Andreoni, Lei Hu, Ariel Amsellem, Ekaterine Dadiani, Tomás Ahumada, Keerthi Kunnumkai, Jake Postiglione, Malte Busmann, Verónica Marín Díaz
article en
15 citations

Abstract

We carried out long-term monitoring of the LIGO/Virgo/KAGRA binary black hole (BBH) merger candidate S230922g in search of electromagnetic emission from the interaction of the merger remnant with an embedding active galactic nuclei (AGN) accretion disk. Using a dataset primarily composed of wide-field imaging from the Dark Energy Camera and supplemented by additional photometric and spectroscopic resources, we searched $\ensuremath{\sim}70%$ of the sky area probability for transient phenomena and discovered six counterpart candidates. One especially promising candidate---AT 2023aagj---exhibited temporally varying asymmetric components in spectral broad line regions, a feature potentially indicative of an off-center event such as a BBH merger. This represents the first live search and multiwavelength, photometric, and spectroscopic monitoring of a gravitational wave BBH optical counterpart candidate in the disk of an AGN.

Physical review. D/Physical review. D.Vol. 110(12)
California Institute of Technology (US), Goddard Space Flight Center (US), American Museum of Natural History (US), City University of New York (US), University of Minnesota System (US), Max Planck Institute for Extraterrestrial Physics (DE), Excellence Cluster Origins (DE), NSF NOIRLab (US), Flatiron Health (United States) (US), Flatiron Institute (US), University of Portsmouth (GB), University of Maryland, College Park (US), Carnegie Mellon University (US), Ludwig-Maximilians-Universität München (DE)
National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Simons Foundation, Stanford University, University of Pennsylvania, Ohio State University, California Institute of Technology, University of Chicago, University of Michigan, Texas A and M University, University of Portsmouth, National Centre for Supercomputing Applications, Higher Education Funding Council for England, Ministarstvo znanosti i obrazovanja, National Energy Research Scientific Computing Center, University of Cambridge, University College London, University of Nottingham, University of Sussex, University of Edinburgh, Deutsche Forschungsgemeinschaft, National Natural Science Foundation of China, Chinese Academy of Sciences, Eidgenössische Technische Hochschule Zürich, Ministério da Ciência, Tecnologia e Inovação, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Financiadora de Estudos e Projetos, Ludwig-Maximilians-Universität München, Institut de Física d'Altes Energies, University of Illinois at Urbana-Champaign, Office of Science, University of California, Santa Barbara, Center for Cosmology and Astroparticle Physics, Ohio State University, Kavli Institute for Cosmological Physics, University of Chicago, Science and Technology Facilities Council, Consejo Superior de Investigaciones Científicas, National Astronomical Observatories, Chinese Academy of Sciences, Division of Astronomical Sciences, High Energy Physics, Integrated Electronics Engineering Center, Binghamton University, Argonne National Laboratory, Fermilab, Lawrence Berkeley National Laboratory, SLAC National Accelerator Laboratory
Openalex Percentile: Top 4%
Pulsars and Gravitational Waves Research
4.97
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