REVERBERATION MAPPING RESULTS FOR FIVE SEYFERT 1 GALAXIES
By C. Grier, B. Peterson, R. Pogge, K. Denney, M. Bentz, P. Martini, S. Sergeev, S. Kaspi, T. Minezaki, Y. Zu and 33 more. 2012
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We present the results from a detailed analysis of photometric and spectrophotometric data on five Seyfert 1 galaxies observed as a part of a recent reverberation mapping program. The data were collected at several observatories over a 140 day span beginning in 2010 August and ending in 2011 January. We obtained high sampling-rate light curves for Mrk 335, Mrk 1501, 3C 120, Mrk 6, and PG 2130+099, from which we have measured the time lag between variations in the 5100 Å continuum and the Hβ broad emission line. We then used these measurements to calculate the mass of the supermassive black hole at the center of each of these galaxies. Our new measurements substantially improve previous measurements of MBH and the size of the broad line-emitting region for four sources and add a measurement for one new object. Our new measurements are consistent with photoionization physics regulating the location of the broad line region in active galactic nuclei.
Subfields: Astronomy and Astrophysics, Instrumentation, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/151bc6b2b7521cc628482f9392f371b152fef596
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Citations in the corpus
- THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: TECHNICAL OVERVIEW (2014, methodology): “To further demonstrate that a detection is possible with as few as ∼15 epochs, we examine the observed LCs for the quasar 3C 120 in Grier et al. (2012).”
- Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. IX. 10 New Observations of Reverberation Mapping and Shortened Hβ Lags (2018, methodology): “…et al. 1993, 1998, 2002, 2004; Kaspi et al. 2000, 2007; Bentz et al. 2008, 2009; Denney et al. 2009; Barth et al. 2011, 2013, 2015; Rafter et al. 2011, 2013; Grier et al. 2012, 2017; Du et al. 2014, 2015, 2016b; Wang et al. 2014a; Jiang et al. 2016; Shen et al. 2016; Fausnaugh et al. 2017).”
- Measuring the Masses of Supermassive Black Holes (2014, background): “…a consortium of astronomers primarily in eastern Europe, Mexico, and Germany (e.g., Shapovalova et al. 2010; Popović et al. 2011; Shapovalova et al. 2012) and by the author’s group of collaborators (Bentz et al. 2006b; Denney et al. 2006; Bentz et al. 2007; Denney et al. 2010; Grier et al. 2012b).”
- THE MAN BEHIND THE CURTAIN: X-RAYS DRIVE THE UV THROUGH NIR VARIABILITY IN THE 2013 ACTIVE GALACTIC NUCLEUS OUTBURST IN NGC 2617 (2013, methodology): “This enables, for example, th reverberation mapping (RM) technique for studying black hole (BH) masses (e.g., Peterson et al. 2004;Grier et al. 2012b,a, 2013b) or measuring time delays in gravitational lenses (e.g. Tewes et al. 2013).”
- A systematic search for changing-look quasars in SDSS (2015, background): “…Schmidt et al. 2012; Ruan et al. 2014), the broad emission lines (BELs) seen in quasar spectra are usually less variable and lagged with respect to the continuum, as seen in reverberation mapping studies (e.g., Clavel et al. 1991; Peterson 1993; Grier et al. 2012; Peterson 2014; Shen et al. 2015).”
- X-ray reverberation around accreting black holes (2014, background): “Such work has culminated in the measurement of black hole masses for a wide range of AGN (e.g. Grier et al. 2012 and see Peterson & Bentz 2006 for a review) and is now leading to the measurement of the detailed structure of the BLR, identifying its inclination to the observer as well as whether the…”
- STELLAR VELOCITY DISPERSION MEASUREMENTS IN HIGH-LUMINOSITY QUASAR HOSTS AND IMPLICATIONS FOR THE AGN BLACK HOLE MASS SCALE (2013, methodology): “The method has since been successfully used to improve RM measurements (Grier et al. 2012; Dietrich et al. 2012) and even recover velocity-delay maps (Grier et al. 2013).”
- THE STRUCTURE OF THE BROAD-LINE REGION IN ACTIVE GALACTIC NUCLEI. I. RECONSTRUCTED VELOCITY-DELAY MAPS (2012, methodology): “Figure 15 shows the model continuum light curve envelope in the bottom panel, and the Hβ light curve from Grier et al. (2012) in the top right panel; the top left panel shows the delay map recovered by MEMECHO.”
- The Sloan Digital Sky Survey Reverberation Mapping Project: Hα and Hβ Reverberation Measurements from First-year Spectroscopy and Photometry (2017, methodology): “Thus far, about 60 AGN have MBH measurements obtained through reverberation mapping (e.g., Peterson et al. 2004; Kaspi et al. 2000, 2005; Bentz et al. 2009, 2010; Denney et al. 2010; Barth et al. 2015; Grier et al. 2012; Du et al. 2014, 2016b,a; Hu et al. 2015).”
- THE LOW-LUMINOSITY END OF THE RADIUS–LUMINOSITY RELATIONSHIP FOR ACTIVE GALACTIC NUCLEI (2013, methodology): “Additional measurements of Hβ radii were de termined for four AGNs in the reverberation sample during a 2010–2011 campaign at MDM and other observatories (Grier et al. 2012; B. M. Peterson et al., in preparation).”
- REVERBERATION MEASUREMENTS OF THE INNER RADIUS OF THE DUST TORUS IN 17 SEYFERT GALAXIES (2014, methodology): “First, we applied widely used, conventional CCF methods that have been employed (White & Peterson 1994; Peterson 2001; Rafter et al. 2011; Barth et al. 2011a,b; Doroshenko et al. 2012; Edri et al 2012; Grier et al. 2012a; Du et al. 2014).”