PKS~J0805$-$0111: A Second Owens Valley Radio Observatory Blazar Showing Highly Significant Sinusoidal Radio Variability -- The Tip of the Iceberg
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2024
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| author | de la Parra, P. V. Kiehlmann, S. Mroz, P. Readhead, A. C. S. Synani, A. Begelman, M. C. Blandford, R. D. Ding, Y. Harrison, F. Liodakis, I. Max-Moerbeck, W. Pavlidou, V. Reeves, R. Vallisneri, M. Aller, M. F. Graham, M. J. Hovatta, T. Lawrence, C. R. Lazio, T. J. W. Mahabal, A. A. Molina, B. O'Neill, S. Pearson, T. J. Ravi, V. Tassis, K. Zensus, J. A. |
| author_facet | de la Parra, P. V. Kiehlmann, S. Mroz, P. Readhead, A. C. S. Synani, A. Begelman, M. C. Blandford, R. D. Ding, Y. Harrison, F. Liodakis, I. Max-Moerbeck, W. Pavlidou, V. Reeves, R. Vallisneri, M. Aller, M. F. Graham, M. J. Hovatta, T. Lawrence, C. R. Lazio, T. J. W. Mahabal, A. A. Molina, B. O'Neill, S. Pearson, T. J. Ravi, V. Tassis, K. Zensus, J. A. |
| contents | Owens Valley Radio Observatory (OVRO) observations of supermassive black hole binary (SMBHB) candidate PKS~2131$-$021 revealed, for the first time, six likely characteristics of the phenomenology exhibited by SMBHB in blazars, of which the most unexpected and critical is sinusoidal flux density variations. We have now identified a second blazar, PKS~J0805$-$0111, showing significant sinusoidal variations, with an observed period that translates to $1.422 \pm 0.005$ yr in the rest frame of the $z = 1.388$ object. We generate $10^6$ simulated light curves to reproduce the radio variability characteristics of PKS~J0805$-$0111, and show that the global probability, considering the \textit{look-elsewhere effect}, indicates that the observed periodicity can be attributed to the red noise tail of the power spectral density, with a $p_0$ value of $7.8 \times 10^{-5}$ (i.e. 3.78$σ$). PKS J0805$-$0111 displays all six characteristics observed in PKS 2131$-$021. Taking into account the well-defined OVRO sample size, the false positive probability $\sim 0.22$, but the rare behavior makes this a strong SMBHB candidate. The discovery of a second SMBHB candidate exhibiting these rare characteristics reveals that PKS~2131$-$021 is not a unique, isolated case. With these two strong cases we are clearly seeing only the tip of the iceberg. We estimate that the number of SMBHB candidates amongst blazars $\sim$ 1 in 100. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2408_02645 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | PKS~J0805$-$0111: A Second Owens Valley Radio Observatory Blazar Showing Highly Significant Sinusoidal Radio Variability -- The Tip of the Iceberg de la Parra, P. V. Kiehlmann, S. Mroz, P. Readhead, A. C. S. Synani, A. Begelman, M. C. Blandford, R. D. Ding, Y. Harrison, F. Liodakis, I. Max-Moerbeck, W. Pavlidou, V. Reeves, R. Vallisneri, M. Aller, M. F. Graham, M. J. Hovatta, T. Lawrence, C. R. Lazio, T. J. W. Mahabal, A. A. Molina, B. O'Neill, S. Pearson, T. J. Ravi, V. Tassis, K. Zensus, J. A. High Energy Astrophysical Phenomena Astrophysics of Galaxies Owens Valley Radio Observatory (OVRO) observations of supermassive black hole binary (SMBHB) candidate PKS~2131$-$021 revealed, for the first time, six likely characteristics of the phenomenology exhibited by SMBHB in blazars, of which the most unexpected and critical is sinusoidal flux density variations. We have now identified a second blazar, PKS~J0805$-$0111, showing significant sinusoidal variations, with an observed period that translates to $1.422 \pm 0.005$ yr in the rest frame of the $z = 1.388$ object. We generate $10^6$ simulated light curves to reproduce the radio variability characteristics of PKS~J0805$-$0111, and show that the global probability, considering the \textit{look-elsewhere effect}, indicates that the observed periodicity can be attributed to the red noise tail of the power spectral density, with a $p_0$ value of $7.8 \times 10^{-5}$ (i.e. 3.78$σ$). PKS J0805$-$0111 displays all six characteristics observed in PKS 2131$-$021. Taking into account the well-defined OVRO sample size, the false positive probability $\sim 0.22$, but the rare behavior makes this a strong SMBHB candidate. The discovery of a second SMBHB candidate exhibiting these rare characteristics reveals that PKS~2131$-$021 is not a unique, isolated case. With these two strong cases we are clearly seeing only the tip of the iceberg. We estimate that the number of SMBHB candidates amongst blazars $\sim$ 1 in 100. |
| title | PKS~J0805$-$0111: A Second Owens Valley Radio Observatory Blazar Showing Highly Significant Sinusoidal Radio Variability -- The Tip of the Iceberg |
| topic | High Energy Astrophysical Phenomena Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2408.02645 |