Publications (16)
GTC Spectra of z ~ 2.3 Quasars: Comparison with Local Luminosity Analogues
Jack W. Sulentic, Paola Marziani, Ascensión del Olmo +3
partly obscured accretion disk model to explain Shifted broad Balmer emission lines of Active Galactic Nuclei
Xue-GUang Zhang, Deborah Dultzin, Ting-Gui Wang +1
Physical Conditions in the Broad Line Region of $z\sim3$ Quasars: A Photoionization Method to Derive $r_{BLR}$
C. Alenka Negrete, Deborah Dultzin, Paola Marziani +1
BLR Physical Conditions in Extreme Population A Quasars: a Method to Estimate Central Black Hole Mass at High Redshift
Alenka Negrete, Deborah Dultzin, Paola Marziani +1
The phylogeny of quasars and the ontogeny of their central black holes
Didier Fraix-Burnet, Paola Marziani, Mauro D 'Onofrio +1
Nuclear Activity In Isolated Galaxies
Francisco Hernandez-Ibarra, Deborah Dultzin, Yair Krongold +3
Low- and high-z highly accreting quasars in the 4D Eigenvector 1 context
Paola Marziani, Jack W. Sulentic, C. Alenka Negrete +4
Induced nuclear activity in galaxy pairs with different morphologies (E+E), (E+S) and (S+S)
Francisco J. Hernández-Ibarra, Yair Krongold, Deborah Dultzin +5
The Correlation Between Spectral Index And Accretion Rate For AGN
Xue-Guang Zhang, Deborah Dultzin, Ting-Gui Wang
OI and CaII observations in intermediate redshift quasars
Mary Loli MartÃnez-Aldama, Deborah Dultzin, Paola Marziani +4
Reverberation and photoionization estimates of the Broad Line Region Radius in Low-z Quasars
C. Alenka Negrete, Deborah Dultzin, Paola Marziani +1
CIV 1549 as an Eigenvector 1 Parameter for Active Galactic Nuclei
Jack W. Sulentic, Rumen Bachev, Paola Marziani +2
Our Search for an H-R Diagram of Quasars
Jack W. Sulentic, Sebastian Zamfir, Paola Marziani +1
Low Ionization Emission Lines in Quasars: Clues from OI 8446 and the CaII Triplet
Paola Marziani, Mary Loli Martinez-Aldama, Deborah Dultzin +1
Low ionization lines in high luminosity quasars: The calcium triplet
Mary Loli MartÃnez-Aldama, Deborah Dultzin, Paola Marziani +4
Circumnuclear star-formation and AGN activity: Clues from surface brightness radial profile of PAHs and [SIV]
Donaji Esparza-Arredondo, Omaira Gonzalez-Martin, Deborah Dultzin +6