Black hole mass estimates based on C IV are consistent with those based on the 
Balmer lines

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.

doi:10.1088/0004-637X/742/2/93

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Black hole mass estimates based on C IV are consistent with those based on the Balmer lines

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Ageorges, N.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Buschkamp, P.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Gemperlein, H.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Hofmann, R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Lederer, R.
MPI for Extraterrestrial Physics, Max Planck Society;

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Assef, R. J., Denney, K. D., Kochanek, C. S., Peterson, B. M., Kozłowski, S., Ageorges, N., et al. (2011). Black hole mass estimates based on C IV are consistent with those based on the Balmer lines. The Astrophysical Journal, 742(2): 93, pp. 1-26. doi:10.1088/0004-637X/742/2/93.

Cite as: https://hdl.handle.net/11858/00-001M-0000-000F-3A51-1

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