Intensive X-ray/UVOIR continuum reverberation mapping of the Seyfert AGN MCG+08-11-11
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| Main Authors: | , , , , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| author | Kynoch, D. McHardy, I. M. Cackett, E. M. Gelbord, J. Santisteban, J. V. Hernández Horne, K. Miller, J. A. Netzer, H. Done, C. Edelson, R. Fausnaugh, M. M. Goad, M. R. Peterson, B. M. Vincentelli, F. M. |
| author_facet | Kynoch, D. McHardy, I. M. Cackett, E. M. Gelbord, J. Santisteban, J. V. Hernández Horne, K. Miller, J. A. Netzer, H. Done, C. Edelson, R. Fausnaugh, M. M. Goad, M. R. Peterson, B. M. Vincentelli, F. M. |
| contents | We present results from intensive (x3 daily), three-month-long X-ray, UV and optical monitoring of the bright Seyfert active galactic nucleus (AGN) MCG+08-11-11 with Swift, supported by optical-infrared ground-based monitoring. The 12 resultant, well-sampled, lightcurves are highly correlated; in particular, the X-ray to UV correlation r_max = 0.85 is, as far as we know, the highest yet recorded in a Seyfert galaxy. The lags increase with wavelength, as expected from reprocessing of central high-energy emission by surrounding material. Our lag spectrum is much shallower than that obtained from an optical monitoring campaign conducted a year earlier when MCG+08-11-11 was approximately 4 times brighter. After filtering out long-term trends in the earlier optical lightcurves we recover shorter lags consistent with our own - demonstrating concurrent reverberation signals from different spatial scales and the luminosity dependence of the measured lags. We use our lag spectrum to test several physical models, finding that disc reprocessing models cannot account for the observed 'excess' lags in the u and r-i-bands that are highly indicative of the Balmer and Paschen continua produced by reprocessing in the broad line region (BLR) gas. The structure seen in both the variable (rms) and lag spectra, and the large time delay between X-ray and UV variations (approximately 2 days) all suggest that the BLR is the dominant reprocessor. The hard X-ray spectrum (Gamma approximately 1.7) and faint, red, UV-optical spectrum both indicate that the Eddington accretion ratio is low: approximately 0.03. The bolometric luminosity then requires that the black hole mass is substantially greater than current reverberation mapping derived estimates. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2511_05342 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Intensive X-ray/UVOIR continuum reverberation mapping of the Seyfert AGN MCG+08-11-11 Kynoch, D. McHardy, I. M. Cackett, E. M. Gelbord, J. Santisteban, J. V. Hernández Horne, K. Miller, J. A. Netzer, H. Done, C. Edelson, R. Fausnaugh, M. M. Goad, M. R. Peterson, B. M. Vincentelli, F. M. Astrophysics of Galaxies We present results from intensive (x3 daily), three-month-long X-ray, UV and optical monitoring of the bright Seyfert active galactic nucleus (AGN) MCG+08-11-11 with Swift, supported by optical-infrared ground-based monitoring. The 12 resultant, well-sampled, lightcurves are highly correlated; in particular, the X-ray to UV correlation r_max = 0.85 is, as far as we know, the highest yet recorded in a Seyfert galaxy. The lags increase with wavelength, as expected from reprocessing of central high-energy emission by surrounding material. Our lag spectrum is much shallower than that obtained from an optical monitoring campaign conducted a year earlier when MCG+08-11-11 was approximately 4 times brighter. After filtering out long-term trends in the earlier optical lightcurves we recover shorter lags consistent with our own - demonstrating concurrent reverberation signals from different spatial scales and the luminosity dependence of the measured lags. We use our lag spectrum to test several physical models, finding that disc reprocessing models cannot account for the observed 'excess' lags in the u and r-i-bands that are highly indicative of the Balmer and Paschen continua produced by reprocessing in the broad line region (BLR) gas. The structure seen in both the variable (rms) and lag spectra, and the large time delay between X-ray and UV variations (approximately 2 days) all suggest that the BLR is the dominant reprocessor. The hard X-ray spectrum (Gamma approximately 1.7) and faint, red, UV-optical spectrum both indicate that the Eddington accretion ratio is low: approximately 0.03. The bolometric luminosity then requires that the black hole mass is substantially greater than current reverberation mapping derived estimates. |
| title | Intensive X-ray/UVOIR continuum reverberation mapping of the Seyfert AGN MCG+08-11-11 |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2511.05342 |