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          Document History for Document ID 448159

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Document Version Version Comment Date Status
448159.0 [No comment] 28.05.2018 16:41 Released

ID: 448159.0, MPI für Astronomie / Publikationen_mpia
Massive galaxies in COSMOS: evolution of black hole versus bulge mass but not versus total stellar mass over the last 9 Gyr?
Authors:Jahnke, Knud; Bongiorno, Angela; Brusa, Marcella; Capak, Peter; Cappelluti, Nico; Cisternas, Mauricio; Civano, Francesca; Colbert, James; Comastri, Andrea; Elvis, Martin; Hasinger, Günther; Ilbert, Olivier; Impey, Chris; Inskip, Katherine; Koekemoer, Anton M.; Lilly, Simon; Maier, Christian; Merloni, Andrea; Riechers, Dominik; Salvato, Mara; Schinnerer, Eva; Scoville, Nick Z.; Silverman, John; Taniguchi, Yoshi; Trump, Jonathan R.; Yan, Lin
Language:English
Date of Publication (YYYY-MM-DD):2009
Title of Journal:The Astrophysical Journal
Journal Abbrev.:ApJ
Volume:706
Start Page:L215
End Page:L220
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:We constrain the ratio of black hole (BH) mass to total stellar mass of type-1 active galactic nuclei (AGNs) in the COSMOS survey at 1 < z < 2. For 10 AGNs at mean redshift z ~ 1.4 with both Hubble Space Telescope (HST)/ACS and HST/NICMOS imaging data, we are able to compute the total stellar mass M *,total, based on rest-frame
Free Keywords:galaxies: active; galaxies: evolution; galaxies: fundamental parameters; galaxies: nuclei
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2009ApJ...706L.215J [ID No:1]