1992
DOI: 10.1086/191661
|View full text |Cite
|
Sign up to set email alerts
|

The emission-line properties of low-redshift quasi-stellar objects

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

106
2,358
15
2

Year Published

2006
2006
2022
2022

Publication Types

Select...
9
1

Relationship

0
10

Authors

Journals

citations
Cited by 1,565 publications
(2,481 citation statements)
references
References 0 publications
106
2,358
15
2
Order By: Relevance
“…We use a theoretical FeII template described in Netzer & Trakhtenbrot (2007) which is based on the Boroson & Green (1992) template and convolve it to fit the spectral resolution of the ESI spectrum. We restrict ourselves to FeII emission in the wavelength range 4900 -5400Å, and rescale the relative amplitude of the template to match the features in our spectrum.…”
Section: Line Profilesmentioning
confidence: 99%
“…We use a theoretical FeII template described in Netzer & Trakhtenbrot (2007) which is based on the Boroson & Green (1992) template and convolve it to fit the spectral resolution of the ESI spectrum. We restrict ourselves to FeII emission in the wavelength range 4900 -5400Å, and rescale the relative amplitude of the template to match the features in our spectrum.…”
Section: Line Profilesmentioning
confidence: 99%
“…AGN powers used in this work are summarised in Table 3. Boroson & Green (1992), Shen & Ho (2014) and Sun & Shen (2015) have found that for a given AGN continuum luminosity radio-loud AGN have higher [OIII] magnitudes or fluxes than radio-quiet AGN as a result of having different Eddington accretion rates. Most of our radio-loud AGN contain LERGs which have different accretion mode than typical AGN.…”
Section: Agn Power Indicatorsmentioning
confidence: 99%
“…5 there). A relation between the He ii EW and the SED may be indicated by the strong relation of He ii EW with the quasar luminosity L (Boroson & Green 1992;Dietrich et al 2002), and the relation between L and the SED (Scott et al 2004;Strateva et al 2005;Steffen et al 2006;Just et al 2007;Stern & Laor 2012;cf. Telfer et al 2002;Shull et al 2012).…”
Section: Similar Relations For the Broad Line Region C Iv Emissionmentioning
confidence: 99%