Phenomenology of Broad Emission Lines in Active Galactic Nuclei

By J. Sulentic, P. Marziani, D. Dultzin-Hacyan. 2000

347 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/bc6392090da2aed9f5e997c7eeb4091289e08c4d

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In Astronomy and Astrophysics

1. D. Schneider
2. Gordon Richards
3. M. Strauss
4. J. Brinkmann
5. Jenny E. Greene
6. Luis C. Ho
7. H. Netzer
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In Nuclear and High Energy Physics

1. D. Schneider
2. Gordon Richards
3. M. Strauss
4. Yue Shen
5. Jenny E. Greene
6. Luis C. Ho
7. J. Brinkmann
8. Xin Liu

Citations in the corpus

• What controls the C iv line profile in active galactic nuclei (2004, result): “Also, Sulentic et al. (2000) suggest there is a significant correlation between the C iv shift/C iv EW ratio and the Hβ FWHM, again this correlation is not significant in our sample.”
• COMPARING SINGLE-EPOCH VIRIAL BLACK HOLE MASS ESTIMATORS FOR LUMINOUS QUASARS (2012, background): “However, the highionization CIV line differs from low-ionization lines such as MgII and the Balmer lines in many ways (for a review, see Sulentic et al. 2000), most notably it shows a prominent blueshift with respect to the low-ionization lines (e.g., Gaskell 1982).”
• What broad emission lines tell us about how active galactic nuclei work (2009, background): “It has been known for over three decades now that object-to-object differences are correlated with each other, and one of main drivers of the correlated differences is the Eddington ratio (see Sulentic et al. 2000 and these proceedings).”
• C IV λ1549 as an Eigenvector 1 Parameter for Active Galactic Nuclei (2007, methodology): “The search for a parameter space that might provide spectroscopic unification for all classes of broad line emitting active galactic nuclei (AGNs) motivated the ‘‘four-dimensional Eigenvector 1’’ (4DE1) concept (Sulentic et al. 2000b, 2000c).”
• Spectral Classification of Quasars in the Sloan Digital Sky Survey: Eigenspectra, Redshift, and Luminosity Effects (2004, background): “Hence, the Baldwin effect is not limited to the C iv emission line and is also observed in many broad emission lines (see, for example, a summary in Sulentic et al. 2000).”
• Broad Emission-Line Shifts in Quasars: An Orientation Measure for Radio-Quiet Quasars? (2002, background): “However, such an effect is not entirely without precedent: see Sulentic et al. (2000); also both Francis & Koratkar (1995) and Corbin & Boroson (1996) found enhanced Baldwin Effects (Baldwin 1977, also see § 4.2) in the red wing of C IV.”
• The origin of the broad line region in active galactic nuclei (2010, background): “However, major uncertainties about the geometry, dynamics, and physics of BLR still remain unknown (for a review, see e.g. Sulentic et al. 2000, Gaskell 2009).”
• UNIFICATION OF LUMINOUS TYPE 1 QUASARS THROUGH C iv EMISSION (2010, background): “Lastly, our results do not disagree that RL quasars are extrema in some sense—rather our results suggest that some RQ quasars do indeed have similar properties (see also Sulentic et al. 2000b).”
• Average Quasar Spectra in the Context of Eigenvector 1 (2002, background): “…P., Sulentic, J. W., Zwitter, T., Dultzin-Hacyan, D., & Calvani, M. 2001, ApJ, 558, 553 [8]Osterbrock, D. E. & Shuder, J. M. 1982, ApJS, 49, 149 [Sulentic et al. 2000a]Sulentic J.W.,Marziani P., Dultzin-Hacyan D., 2000a, AR A&A, 38, 521 [9]Sulentic, J. W., Zwitter, T., Marziani, P., &…”
• Biases in Virial Black Hole Masses: An SDSS Perspective (2007, background): “Thus it is important to study these broad lines simultaneously with multiband spectra (e.g., Sulentic et al. 2000 and references therein; Baskin & Laor 2005).”
• A Systematic Analysis of Fe II Emission in Quasars: Evidence for Inflow to the Central Black Hole (2008, methodology): “The Physical Driver of vFe The Eddington ratio Lbol/LEdd is often suggested to be the main physical driver of the spectral diversity in quasars (Sulentic et al. 2000a, 2000b; Marziani et al. 2001, 2003a; Boroson 2002), and MBH is argued to be an important determinant of radioloudness (Laor 2000;…”
• Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. IX. 10 New Observations of Reverberation Mapping and Shortened Hβ Lags (2018, background): “Principal component analysis has revealed that the main variance of quasar optical spectra is a strong correlation between the flux ratio of broad Fe IIto Hβ emission, the strength of [O III] λ5007, and the width of Hβ (Boroson & Green 1992; Sulentic et al. 2000a).”
• An Optical Spectroscopic Atlas of Low-Redshift Active Galactic Nuclei (2003, methodology): “Exceptions are few although notable (e.g., Sulentic et al. 2000b).”