Deborah Dultzin Kessler
Dultzin-Hacyan, Déborah 1945-...
Dultzin, Déborah
VIAF ID: 41893104 (Personal)
Permalink: http://viaf.org/viaf/41893104
Preferred Forms
- 100 0 _ ‡a Deborah Dultzin Kessler
- 100 1 _ ‡a Dultzin, Déborah
- 200 _ | ‡a Dultzin-Hacyan ‡b Déborah ‡f 1945-....
- 100 1 _ ‡a Dultzin-Hacyan, Déborah ‡d 1945-...
4xx's: Alternate Name Forms (12)
Works
Title | Sources |
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Activity induced by gravitational interaction in galaxy pairs | |
Activity of the Seyfert galaxy neighbours | |
AGILE detection of a rapid γ-ray flare from the blazar PKS 1510-089 during the GASP-WEBT monitoring | |
The broad line region of quasars | |
C IV {lambda}1549 as an Eigenvector 1 parameter for active galactic nuclei | |
Circumnuclear Star Formation and AGN Activity: Clues from Surface Brightness Radial Profile of PAHs and [${\rm{S}}\,{\rm{IV}}$] | |
The correlation between spectral index and accretion rate for AGN | |
Detailed characterization of H{beta} emission line profile in low-z SDSS quasars | |
The dust geometric distribution in Seyfert 1 and Seyfert 2 galaxies, isolated and in interaction | |
Early Science with the Large Millimeter Telescope: An Energy-driven Wind Revealed by Massive Molecular and Fast X-Ray Outflows in the Seyfert Galaxy IRAS 17020+4544 | |
Editorial: Quasars at All Cosmic Epochs | |
The environment of Sy1, Sy2 and bright IRAS galaxies: the AGN/starburst connection | |
Extreme Quasars as Distance Indicators in Cosmology | |
From Observations to Physical Parameters | |
The GASP-WEBT monitoring of 3C 454.3 during the 2008 optical-to-radio and γ-ray outburst | |
GTC spectra of z =~ 2.3 quasars: comparison with local luminosity analogs | |
HE0359-3959: An Extremely Radiating Quasar | |
Highly accreting quasars: The SDSS low-redshift catalog | |
Hints on the Gradual Resizing of the Torus in AGNs through Decomposition of Spitzer/IRS Spectra | |
O I and Ca II observations in intermediate redshift quasars | |
The incidence of nuclear activity in galaxy pairs with different morphologies (E+E), (E+S) and (S+S) | |
Long-term variability of the optical spectra of NGC4151. I. Light curves and flux correlations | |
A Main Sequence for Quasars | |
MULTIWAVELENGTH OBSERVATIONS OF 3C 454.3. III. EIGHTEEN MONTHS OFAGILEMONITORING OF THE “CRAZY DIAMOND” | |
Multiwavelength observations of a TeV-flare from W Comae | |
Nuclear obscuration in LINERs. Clues from Spitzer/IRS spectra on the Compton thickness and the existence of the dusty torus | |
Observations of the first electromagnetic counterpart to a gravitational-wave source by the TOROS Collaboration | |
On the interpretation of the He II lambda 4686 emission line in HDE 226868 (Cygnus X-1) | |
Partly obscured accretion disc model to explain shifted broad Balmer emission lines of active galactic nuclei | |
A photo-ionization method for black hole mass estimation in quasars | |
The Phylogeny of Quasars and the Ontogeny of Their Central Black Holes | |
Polarimetric monitoring of blazars at San Pedro Martir | |
Quasar Massive Ionized Outflows Traced by CIV λ1549 and [OIII]λλ4959,5007 | |
Quasars as Cosmological Standard Candles | |
Quasars Classes and Their Relationships | |
Quasars in the Cosmic Environment | |
Quasars: The Observational Perspectives | |
THE SPECTRAL ENERGY DISTRIBUTION OFFERMIBRIGHT BLAZARS | |
Spectral microvariability in quasars | |
Spectral optical monitoring of a double-peaked emission line AGN Arp 102B. Variability of spectral lines and continuum | |
Spectral optical monitoring of the narrow-line Seyfert 1 galaxy Ark 564 | |
Spectrophotométrie des noyaux actifs des galaxies | |
Studying the evolution of galaxies in compact groups over the past 3 Gyr – II. The importance of environment in the suppression of star formation | |
VAMOS: A pathfinder for the HAWC gamma-ray observatory | |
WEBT multiwavelength monitoring and XMM-Newton observations of BL Lacertae in 2007-2008. Unveiling different emission components | |
What does CIV{lambda}1549 tell us about the physical driver of the Eigenvector quasar sequence? | |
X-ray long-term variations in the low-luminosity AGN NGC 835 and its circumnuclear emission |