We present the discovery of a Baldwin effect in 8 nearby Seyfert galaxies for the three most prominent mid-infrared forbidden emission lines observable from the ground that are commonly found in AGN, [AR II
<p>The origin of the unification model for AGN was the detection of broad hydrogen recombination lin...
The existence of an anti-correlation between the equivalent width (EW) of the narrow core ...
The luminosity dependence of the equivalent width of CIV in active galaxies, the "Baldwin" effect, i...
We present the discovery of a Baldwin effect in 8 nearby Seyfert galaxies for the three most promine...
International audienceWe present our discovery of a narrow-line Baldwin effect, an anticorrelation b...
We investigate the intrinsic Baldwin effect (Beff) of the broad Hα and Hβ emission lines for six Typ...
We present our discovery of a narrow-line Baldwin effect, an anticorrelation between the equivalent ...
The origin of the luminosity dependence of the strength of broad and narrow emission lines in AGN (i...
The anti-correlations between the equivalent widths of emission lines and the continuum luminosity i...
The majority of active galactic nuclei (AGN) observed by XMM–Newton reveal narrow Fe Kα lines at ∼6....
Context.The relationship between the emission-line equivalent width and the continuum luminosity, ca...
This review addresses the current observational status of the Baldwin Effect (BE), an empirical anti...
This article tests whether the modified Baldwin effect remains strong across the wides possible of r...
A well investigated phenomenon in the study of Active Galactic Nuclei (AGN) is that of the Broad-Lin...
International audienceThe existence of an anti-correlation between the equivalent width (EW) of the ...
<p>The origin of the unification model for AGN was the detection of broad hydrogen recombination lin...
The existence of an anti-correlation between the equivalent width (EW) of the narrow core ...
The luminosity dependence of the equivalent width of CIV in active galaxies, the "Baldwin" effect, i...
We present the discovery of a Baldwin effect in 8 nearby Seyfert galaxies for the three most promine...
International audienceWe present our discovery of a narrow-line Baldwin effect, an anticorrelation b...
We investigate the intrinsic Baldwin effect (Beff) of the broad Hα and Hβ emission lines for six Typ...
We present our discovery of a narrow-line Baldwin effect, an anticorrelation between the equivalent ...
The origin of the luminosity dependence of the strength of broad and narrow emission lines in AGN (i...
The anti-correlations between the equivalent widths of emission lines and the continuum luminosity i...
The majority of active galactic nuclei (AGN) observed by XMM–Newton reveal narrow Fe Kα lines at ∼6....
Context.The relationship between the emission-line equivalent width and the continuum luminosity, ca...
This review addresses the current observational status of the Baldwin Effect (BE), an empirical anti...
This article tests whether the modified Baldwin effect remains strong across the wides possible of r...
A well investigated phenomenon in the study of Active Galactic Nuclei (AGN) is that of the Broad-Lin...
International audienceThe existence of an anti-correlation between the equivalent width (EW) of the ...
<p>The origin of the unification model for AGN was the detection of broad hydrogen recombination lin...
The existence of an anti-correlation between the equivalent width (EW) of the narrow core ...
The luminosity dependence of the equivalent width of CIV in active galaxies, the "Baldwin" effect, i...
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