activity
20202026
most citedThe flux ratio of the [N II] 6548, 6583 Å lines in sample of Active Galactic Nuclei Type 2

35 citations · 114 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

A Meta-Learning Framework for Multitask Reverberation Mapping in Active Galactic Nuclei

Aman N. Raju, Andjelka B. Kovačević, Dragana Ilić +8

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) is expected to observe active galactic nuclei (AGN) at sky densities of approximately 1000-4000 per sq. deg, en…

astro-ph.GA2026

Unravelling the complex structure of the Fe II emission region in Type 1 active galactic nuclei

Jelena Kovačević-Dojčinović, Ivan Dojčinović, Luka Č. Popović

Using a large sample of Type 1 AGN spectra, we investigated the complex structure of the Fe II emission region in order to understand the atomic processes responsible for the enhan…

astro-ph.HE2025★ 3 cited

Multiband optical variability on diverse timescales of the blazar Ton 599 from 2011 to 2023

O. Vince, C. M. Raiteri, M. Villata +72

(Shortened)Context: We analyze the optical variability of the FSRQ Ton 599 using BVRI photometry from the WEBT collaboration (2011-2023), complemented by photometric and spectrosco…

astro-ph.GA2025

AGN STORM 2. XI. Spectroscopic reverberation mapping of the hot dust in Mrk 817

Hermine Landt, Benjamin D. Boizelle, Michael S. Brotherton +41

The AGN Space Telescope and Optical Reverberation Mapping 2 (STORM 2) campaign targeted Mrk 817 with intensive multi-wavelength monitoring and found its soft X-ray emission to be s…

astro-ph.GA2025

Continuum Reverberation Mapping of Accretion Disks Surrounding Supermassive Black Hole Binaries: Observational Signatures

Yi-Xin Fu, Yan-Rong Li, Jian-Min Wang +9

It has remained challenging to reliably identify sub-parsec supermassive black hole binaries (SMBHBs), despite them being expected to be ubiquitous. We propose a new method using m…

astro-ph.GA2025

The Intermediate-Mass Black Hole Reverberation Mapping Project: First Detection of Mid-Infrared Lags in Prototypical IMBHs in NGC 4395 and POX 52

Jingbo Sun, Hengxiao Guo, Wenwen Zuo +25

The search for robust evidence of intermediate-mass black holes (IMBHs) is crucial for understanding black hole seeding process and the formation of supermassive black holes in the…

astro-ph.GA2025★ 4 cited

Searching for signatures of Fe II atomic processes in spectra of active galactic nuclei

Jelena Kovačević-Dojčinović, Ivan Dojčinović, Maša Lakićević +1

We use a sample of Type 1 active galactic nuclei (AGNs) spectra in order to investigate which atomic processes are responsible for some observed properties of the FeII emission lin…

astro-ph.GA2025★ 3 cited

Time Evolution of Mg II in SDSS J2320+0024: Implications for a Subparsec Binary Supermassive Black Hole System

Marta Fatović, Dragana Ilić, Andjelka B. Kovačević +8

Here we present results from our spectroscopic follow-up of SDSS J2320+0024, a candidate binary supermassive black hole (SMBH) with a suspected sub-pc separation, identified by a 2…

astro-ph.HE2024

IceCube AGN Neutrino candidate PKS 1717+177: Dark deflector bends nuclear jet

S. Britzen, A. B. Kovačević, M. Zajaček +8

The BL Lac Object PKS 1717+177 has been identified as potential neutrino-emitting AGN in the point source stacking analysis of IceCube data. We explore peculiarities in the morphol…

astro-ph.HE2024★ 20 cited

AGN STORM 2. VII. A Frequency-resolved Map of the Accretion Disk in Mrk 817: Simultaneous X-ray Reverberation and UVOIR Disk Reprocessing Time Lags

Collin Lewin, Erin Kara, Aaron J. Barth +35

X-ray reverberation mapping is a powerful technique for probing the innermost accretion disk, whereas continuum reverberation mapping in the UV, optical, and infrared (UVOIR) revea…

astro-ph.HE2024

AGN STORM 2: IX. Studying the Dynamics of the Ionized Obscurer in Mrk 817 with High-resolution X-ray Spectroscopy

Fatima Zaidouni, Erin Kara, Peter Kosec +45

We present the results of the XMM-Newton and NuSTAR observations taken as part of the ongoing, intensive multi-wavelength monitoring program of the Seyfert 1 galaxy Mrk 817 by the…

astro-ph.GA2023★ 6 cited

Influence of the optical Fe II quasi-continuum on measuring the spectral parameters of active galactic nuclei

Luka Č. Popović, Jelena Kovačević-Dojčinović, Ivan Dojčinović +1

We explore the influence of optical Fe II quasi-continuum on the measured spectral parameters in the 4150-5500 A range for the spectra of Type 1 active galactic nuclei (AGNs). We a…

astro-ph.GA2023★ 3 cited

Polarimetric Reverberation Mapping in Medium-Band Filters

Elena Shablovinskaya, Luka Č. Popović, Roman Uklein +8

Earlier, we suggested the "reload" concept of the polarimetric reverberation mapping of active galactic nuclei (AGN), proposed for the first time more than 10 years ago. We have su…

astro-ph.GA2022★ 35 cited

The flux ratio of the [N II] 6548, 6583 Å lines in sample of Active Galactic Nuclei Type 2

Ivan Dojčinović, Jelena Kovačević-Dojčinović, Luka Č. Popović

In spectra of the Active Galactic Nuclei (AGNs), the [N II] 6548, 6583 A lines are commonly fitted using the fixed intensity ratio of these two lines (R[N II]=I/I…

astro-ph.GA2022★ 7 cited

Spectropolarimetry and spectral decomposition of high-accreting Narrow Line Seyfert 1 galaxies

Marzena Śniegowska, Swayamtrupta Panda, Bożena Czerny +7

Narrow Line Seyfert 1 (NLSy1) galaxies have been shown to have high Eddington ratios and relatively small black hole masses. The measurement of the black hole masses is based on th…

astro-ph.GA2021★ 3 cited

AGN orientation through the spectroscopic correlations and model of dusty cone shell

Maša Lakićević, Jelena Kovačević-Dojčinović, Luka Č. Popović

The differences between Narrow Line Seyfert 1 galaxies (NLS1s) and Broad Line AGNs (BLAGNs) are not completely understood; it is thought that they may have different inclinations a…

astro-ph.HE2021★ 14 cited

Detecting subparsec super-massive binary black holes: Long termmonitoring perspective

Luka Č. Popović, Saša Simić, Anđelka Kovačević +1

Here we consider the perspective to detect sub-pc super-massive binary black-hole (SMBBH) systems using long-term photometric and spectroscopic monitoring campaigns of active galac…

astro-ph.GA2020★ 16 cited

Estimating supermassive black hole masses in AGNs using polarization of broad MgII, H and H lines

Đorđe Savić, Luka Č. Popović, Elena Shablovinskaya +1

For type-1 active galactic nuclei (AGNs) for which the equatorial scattering is the dominant broad line polarization mechanism, it is possible to measure the supermassive black hol…