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Can we improve CIV-based single-epoch black hole mass estimations?
(Oxford University Press, 2018)
In large optical surveys at high redshifts (z > 2), the C IV λ1549 broad emission line is the most
practical alternative to estimate the mass (MBH) of active supermassive black holes. However,
mass determinations obtained ...
Reverberation Mapping of Luminous Quasars at High z
(2018)
We present reverberation mapping (RM) results for 17 high-redshift, high-luminosity quasars with good-quality R-band and emission-line light curves. We are able to measure statistically significant lags for Lyα (11 objects), ...
Compatibility of the large quasar groups with the concordance cosmological model
(2016)
We study the compatibility of large quasar groups with the concordance cosmological model. Large quasar groups are very large spatial associations of quasars in the cosmic web, with sizes of 50-250 h(-1) Mpc. In particular, ...
Dust in the Wind of Quasar PG2112+059
(Spitzer Space Telescope, 2016)
Dust in the Wind of Quasar PG2112+059
(Spitzer Space Telescope, 2011)
Photometric classification of quasars from RCS-2 using Random Forest
(EDP Sciences, 2015)
The classification and identification of quasars is fundamental to many astronomical research areas. Given the large volume of photometric
survey data available in the near future, automated methods for doing so are ...
Photometric classification of quasars from RCS-2 using Random Forest
(EDP Sciences, 2015)
The classification and identification of quasars is fundamental to many astronomical research areas. Given the large volume of photometric survey data available in the near future, automated methods for doing so are required. ...
Photometric classification of quasars from RCS-2 using Random Forest
(EDP Sciences, 2015-12)
The classification and identification of quasars is fundamental to many astronomical research areas. Given the large volume of photometric survey data available in the near future, automated methods for doing so are required. ...
Broad emission-line shifts in quasars: an orientation measure for radio-quiet quasars?
(AMERICAN INSTITUTE OF PHYSICS, 2002)