Lag-Luminosity Relationship for Interband Lags between Variations in B, V, R, and I Bands in Active Galactic Nuclei

By S. Sergeev, V. Doroshenko, Yu. V. Golubinskiy, N. Merkulova, E. Sergeeva. 2005

147 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/e9a3f86068025a5031647bbba4857d17195ab350

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In Aerospace Engineering

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Citations in the corpus

• SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. II. SWIFT AND HST REVERBERATION MAPPING OF THE ACCRETION DISK OF NGC 5548 (2015, unknown): “Ground-based multicolor optical/IR studies also yielded tentative evidence of shorter wavelength variations leading longer wavelength variations in some AGN (Sergeev et al. 2005, Cackett et al. 2007, Lira et al. 2011).”
• Testing thermal reprocessing in active galactic nuclei accretion discs (2007, methodology): “With interband time delays and long-term monitoring lightcurves for 14 AGN, the Sergeev et al. (2005) data offer an opportunity to test this reprocessing model and to determine distances to a sample of 14 AGN.”
• REVERBERATION MAPPING RESULTS FOR FIVE SEYFERT 1 GALAXIES (2012, background): “See Sergeev et al. (2005) for more details on obtaining the CrAO photometric fluxes.”
• REVERBERATION MAPPING MEASUREMENTS OF BLACK HOLE MASSES IN SIX LOCAL SEYFERT GALAXIES (2010, methodology): “For further details of the CrAO V -band observations and reduction, see the similar analysis described by Sergeev et al. (2005).”
• QUANTIFYING QUASAR VARIABILITY AS PART OF A GENERAL APPROACH TO CLASSIFYING CONTINUOUSLY VARYING SOURCES (2009, background): “…function with greater variability amplitudes on longer time baselines (e.g., Vanden Berk et al. 2004; de Vries et al. 2005), and this has also been observed for smaller numbers of individually monitored quasars (e.g., Curti et al. 1985; Nelson 1996; Collin et al. 2002; Sergeev et al. 2005).”
• A systematic search for changing-look quasars in SDSS (2015, background): “…the optical continuum variability is driven at least in part by reprocessing of EUV or X-ray light (e.g., c© 2015 The Authors Collier et al. 1998; Sergeev et al. 2005; Cackett et al. 2007; Shappee et al. 2014; Edelson et al. 2015) but this may be due to inner cloud reprocessing rather than the…”
• THE MAN BEHIND THE CURTAIN: X-RAYS DRIVE THE UV THROUGH NIR VARIABILITY IN THE 2013 ACTIVE GALACTIC NUCLEUS OUTBURST IN NGC 2617 (2013, background): “Lags between shorter- and longer-wavelength continuum variations have been detected in several sources (e.g., Sergeev et al. 2005; Cackett et al. 2007) at marginal significance, and always in the sense that the short-wavelength variations lead those at longer wavelengths.”