activity
20172026
most citedA possible mechanism for multiple changing look phenomenon in Active Galactic Nuclei

135 citations · 996 across the 47 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

28 papers · 1 filter

astro-ph.GA2026

Spatially resolved optical and mid-infrared spectroscopy of SDSS1335+0728: implications for the origin of the Ansky event

P. Sánchez-Sáez, M. Masterson, L. Hernández-García +25

The galaxy SDSS1335+0728 brightened abruptly in December 2019 (the Ansky event) and has since been confirmed as the host of extreme X-ray quasi-periodic eruptions (QPEs) of debated…

astro-ph.GA2026

Radiation Pressure Instability in the "turn-on" Changing-Look AGN SDSS J1430+2303

Han He, Bei You, Marzena Śniegowska +3

We aim to investigate the multi-wavelength variability, spectral, and timing properties of the changing-look active galactic nucleus (CL AGN) SDSS J1430+2303, and to explore the ph…

astro-ph.GA2025

Feeding frenzy in the mighty black holes: what we could learn from them?

Swayamtrupta Panda, Hygor Benati Gonçalves, Thaisa Storchi-Bergmann +14

Eddington ratio is a paramount parameter governing the accretion history and life cycles of Active Galactic Nuclei (AGNs). This short review presents a multi-faceted view of the im…

astro-ph.GA2025

SDSS-V Black Hole Mapper: The Index Diagram as a tool to disentangle the influence of the Host Galaxy in Quasar spectra

C. A. Negrete, R. Sandoval-Orozco, H. Ibarra-Medel +32

We revisit the Quasar Main Sequence (QMS) by investigating the impact of the stellar component from the host galaxy (HG) on the emission line spectra of the active galactic nuclei…

astro-ph.GA2025★ 8 cited

The Nineteenth Data Release of the Sloan Digital Sky Survey

SDSS Collaboration, Gautham Adamane Pallathadka, Mojgan Aghakhanloo +210

Mapping the local and distant Universe is key to our understanding of it. For decades, the Sloan Digital Sky Survey (SDSS) has made a concerted effort to map millions of celestial…

astro-ph.GA2024★ 17 cited

Chemical abundances along the quasar main sequence

A. Floris, P. Marziani, S. Panda +5

The 4D eigenvector 1 (E1) sequence has emerged as a powerful tool for organizing the observational and physical characteristics of type-1 active galactic nuclei (AGNs). In this stu…

astro-ph.GA2024

From sub-solar to super-solar chemical abundances along the quasar main sequence

Paola Marziani, Alberto Floris, Alice Deconto-Machado +8

The 4D Eigenvector 1 sequence has proven to be a highly effective tool for organizing observational and physical properties of type 1 active galactic nuclei (AGN). In this paper, w…

astro-ph.GA2024★ 50 cited

Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results

Grisha Zeltyn, Benny Trakhtenbrot, Michael Eracleous +32

"Changing-look" active galactic nuclei (CL-AGNs) challenge our basic ideas about the physics of accretion flows and circumnuclear gas around supermassive black holes. Using first-y…

astro-ph.GA2023

Accretion processes onto black holes: theoretical problems, observational constraints

Bozena Czerny, Marzena Sniegowska, Agnieszka Janiuk +1

We shortly summarize the standard current knowledge on the structure of the accretion flow onto black holes in galactic binary systems and in active galactic nuclei. We stress the…

astro-ph.GA2023★ 12 cited

Broad-line region in active galactic nuclei: Dusty or dustless?

Ashwani Pandey, Bozena Czerny, Swayamtrupta Panda +5

Context. Dust in active galactic nuclei is clearly present right outside the broad-line region (BLR) in the form of a dusty molecular torus. However, some models of the BLR predict…

astro-ph.GA2023★ 9 cited

UV Fe II emission model of HE 0413-4031 and its relation to broad-line time delays

Michal Zajaček, Swayamtrupta Panda, Ashwani Pandey +11

Fe II emission is a well-known contributor to the UV spectra of active galactic nuclei and the modeling of this part may affect the results obtained for the MgII emiss…

astro-ph.GA2023

BAL effect in quasars due to source orientation

M. Sniegowska, M. H. Naddaf, M. L. Martinez-Aldama +3

We investigated a scenario where the presence of a broad absorption line (BAL) feature in quasars (QSOs) is contingent upon the line of sight being situated within an outflow cone…

astro-ph.GA2023★ 13 cited

Wavelength-resolved reverberation mapping of intermediate redshift quasars HE 0413-4031 and HE 0435-4312: Dissecting Mg II, optical Fe II, and UV Fe II emission regions

Raj Prince, Michal Zajaček, S. Panda +24

We present the wavelength-resolved reverberation mapping (RM) of combined MgII and UV FeII broad-line emissions for two intermediate redshifts (z1), luminous quasars - HE 041…

astro-ph.GA2022★ 19 cited

Dust-driven wind as a model of Broad Absorption Line quasars

Mohammad Hassan Naddaf, Mary Loli Martinez-Aldama, Paola Marziani +3

We test a scenario claiming that the broad absorption line (BAL) phenomenon in quasars (QSOs) is not a temporary stage of their life. In this scenario, we see the BAL effect only i…

astro-ph.GA2022★ 13 cited

Dusty plasma in active galactic nuclei

Bożena Czerny, Michal Zajaček, Mohammad-Hassan Naddaf +10

Since many years we know that dust in the form of the dusty-molecular torus is responsible for the obscuration in active galactic nuclei (AGN) at large viewing angles and thus for…

astro-ph.GA2022★ 22 cited

Accretion disks, quasars and cosmology: meandering towards understanding

Bozena Czerny, Shulei Cao, Vikram Kumar Jaiswal +11

As Setti & Woltjer noted back in 1973, quasars could be used to construct the Hubble diagram but the actual application was not that straightforward. It took years to implement the…

astro-ph.GA2022★ 21 cited

High Metal Content of Highly Accreting Quasars: Analysis of an Extended Sample

Karla Garnica, C. Alenka Negrete, Paola Marziani +3

We present an analysis of UV spectra of quasars at intermediate redshifts believed to belong to the extreme Population A (xA), aimed to estimate the chemical abundances of the broa…

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.GA2022★ 12 cited

Wavelength-resolved Reverberation Mapping of quasar CTSC30.10: Dissecting MgII and FeII emission regions

Raj Prince, Michal Zajaček, Bożena Czerny +20

We present the results of the reverberation monitoring aimed at MgII broad line and FeII pseudocontinuum for the luminous quasar CTS C30.10 (z = 0.90052) with the Southern African…

astro-ph.GA2021★ 11 cited

Linear Spectropolarimetric Analysis of Fairall 9 with VLT/FORS2

Bo-Wei Jiang, Paola Marziani, Đorđe Savić +10

The quasar Main Sequence (MS) appears to be an incredibly powerful tool to organize the diversity in large samples of type-1 quasars but the most important physical parameters gove…

astro-ph.GA2020★ 45 cited

Time Delay of MgII Emission Response for the Luminous Quasar HE 0435-4312: Towards Application of High-Accretor Radius-Luminosity Relation in Cosmology

Michal Zajaček, Bożena Czerny, Mary Loli Martinez-Aldama +21

Using the six years of the spectroscopic monitoring of the luminous quasar HE 0435-4312 () with the Southern African Large Telescope (SALT), in combination with the photo…

astro-ph.GA2020★ 135 cited

A possible mechanism for multiple changing look phenomenon in Active Galactic Nuclei

M. Sniegowska, B. Czerny, E. Bon +1

Changing-look phenomenon observed now in a growing number of active galaxies challenges our understanding of the accretion process close to a black hole. We propose a simple explan…

astro-ph.GA2020★ 44 cited

Time-delay measurement of MgII broad line response for the highly-accreting quasar HE 0413-4031: Implications for the MgII-based radius-luminosity relation

Michal Zajaček, Bożena Czerny, Mary Loli Martinez-Aldama +16

We present the monitoring of the AGN continuum and MgII broad line emission for the quasar HE 0413-4031 () based on the six-year monitoring by the South African Large Teles…

astro-ph.GA2019★ 12 cited

Mechanism of the Changing Look phenomenon in Active Galactic Nuclei

Marzena Śniegowska, Bożena Czerny

Changing-look phenomenon observed now in a growing number of active galaxies challenges our understanding of the accretion process close to a black hole. We propose a simple explan…