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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 607597.0, MPI für Astronomie / Publikationen_mpia
Black hole mass estimates based on C IV are consistent with those based on the Balmer lines
Authors:Assef, R. J.; Denney, K. D.; Kochanek, C. S.; Peterson, B. M.; Kozłowski, S.; Ageorges, N.; Barrows, R. S.; Buschkamp, P.; Dietrich, M.; Falco, E.; Feiz, C.; Gemperlein, H.; Germeroth, A.; Grier, C. J.; Hofmann, R.; Juette, M.; Khan, R.; Kilic, M.; Knierim, V.; Laun, W.; Lederer, R.; Lehmitz, M.; Lenzen, R.; Mall, U.; Madsen, K. K.; Mandel, H.; Martini, P.; Mathur, S.; Mogren, K.; Mueller, P.; Naranjo, V.; Pasquali, A.; Polsterer, K.; Pogge, R. W.; Quirrenbach, A.; Seifert, W.; Stern, D.; Shappee, B.; Storz, C.; Van Saders, J.; Weiser, P.; Zhang, D.
Date of Publication (YYYY-MM-DD):2011
Journal Abbrev.:The Astrophysical Journal
Volume:742
Issue / Number:2
Audience:Not Specified
Abstract / Description:Using a sample of high-redshift lensed quasars from the CASTLES project with observed-frame ultraviolet or optical and near-infrared spectra, we have searched for possible biases between supermassive black hole (BH) mass estimates based on the C IV, Hα, and Hβ broad emission lines. Our sample is based upon that of Greene, Peng, & Ludwig, expanded with new near-IR spectroscopic observations, consistently analyzed high signal-to-noise ratio (S/N) optical spectra, and consistent continuum luminosity estimates at 5100 Ã…. We find that
Free Keywords:galaxies: active; gravitational lensing: strong; quasars: emission lines
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://cdsads.u-strasbg.fr/abs/2011ApJ...742...93A
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