activity
20062013
most citedAnalysis of optical Fe II emission in a sample of AGN spectra

207 citations · 557 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2013★ 25 cited

A model for the Balmer pseudocontinuum in spectra of type 1 AGNs

Jelena Kovacevic, Luka C. Popovic, Wolfram Kollatschny

Here we present a new method for subtracting the Balmer pseudocontinuum in the UV part of type 1 AGN spectra. We calculate the intensity of the Balmer pseudocontinuum using the pro…

astro-ph.CO2013★ 2 cited

Spectral properties of a sample of type 1 AGNs: influence of star formation

Luka C. Popovic, Jelena Kovacevic, Milan S. Dimitrijevic

To find the spectral properties of AGNs in optical spectral band (around the Hb line) we constructed an Fe II template, that is covering Fe II emission from 4100 A to 5600 A. Using…

astro-ph.CO2012★ 100 cited

Spectral Optical Monitoring of the Narrow Line Seyfert 1 galaxy Ark 564

A. I. Shapovalova, L. C. Popovic, A. N. Burenkov +14

We present the results of a long-term (1999--2010) spectral optical monitoring campaign of the active galactic nucleus (AGN) Ark 564, which shows a strong Fe II line emission in th…

astro-ph.CO2012★ 2 cited

Spectral monitoring of AGNs: Preliminary results for Ark 564 and Arp 102B

A. I. Shapovalova, L. C. Popovic, D. Ilic +4

We present preliminary results of the long term spectral monitoring of two active galactic nuclei with different broad line shapes: Ark 564 and Arp 102B. Ark 564 is a bright nearby…

astro-ph.GA2011★ 33 cited

Photo-centric variability of quasars caused by variations in their inner structure: Consequences on Gaia measurements

Luka C. Popovic, Predrag Jovanovic, Marko Stalevski +4

We study the photocenter position variability due to variations in the quasar inner structure. We consider variability in the accretion disk emissivity and torus structure variabil…

astro-ph.CO2011★ 22 cited

Optical emission line properties of a sample of the broad-line AGNs: the Baldwin effect and eigenvector 1

Luka C. Popovic, Jelena Kovacevic

We divide a sample of 302 type-1 AGNs into two subsamples based on the narrow line [OIII]/Hbeta_{NLR} ratio, since we expect that there will be a stronger starburst (HII region) co…