Highly accreting quasars: a tool for cosmology?
Date Issued
2017
Author(s)
•
Negrete, C. A.
•
Dultzin, D.
•
Martinez-Aldama, M. L.
•
Del Olmo, A.
•
Esparza, D.
•
Sulentic, J. W.
•
D'Onofrio, M.
•
•
Bon, E.
•
Bon, N.
Abstract
Highly accreting quasars are possible cosmological probes, as their Eddington ratio is expected to saturate toward values of order unity. We present preliminary estimates of redshift- independent source luminosities and the Hubble diagram for quasars in the redshift range 0.1 <~ z <~ 2.6.
Coverage
New Frontiers in Black Hole Astrophysics
All editors
Gomboc, Andreja
Volume
vol. 12, S324
Start page
245
Conferenece
New Frontiers in Black Hole Astrophysics
Conferenece place
Ljubljana, Slovenia
Conferenece date
12-16 September, 2016
Issn Identifier
1743-9213
Ads BibCode
2017IAUS..324..245M
Rights
open.access
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