collaborators

7 papers

astro-ph.GA2025

Evidence for a Stratified Accretion Disk Wind in AGN

P. Marziani, E. Bon, S. Panda +5

We present observational evidence supporting the presence of a stratified accretion disk wind in active galactic nuclei (AGN), based on multi-wavelength spectroscopic analysis of b…

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

The spectral energy distribution of extreme population A quasars

Karla Garnica, Deborah Dultzin, Paola Marziani +1

Knowledge of the broad-band active galactic nuclei (AGN) spectral energy distribution (SED) that ionizes the gas-rich broad emission line region is key to understanding the various…

astro-ph.GA2025

LBT IR observations of candidate super-Eddington quasars

T. M. Buendia-Rios, P. Marziani, C. A. Negrete +1

Quasars accreting at very high rates are believed to be prime movers of galactic evolution because of their high radiative and mechanical output. The study presented in this paper…

astro-ph.GA2025

The properties of the obscuring material of an AGNs sample from mid-IR and X-ray simultaneous fitting

Donaji Esparza-Arredondo, Omaira Gonzalez-Martín, Deborah Dultzin +5

Over ten mid-infrared (mid-IR) and X-ray models are currently attempting to describe the nuclear obscuring material of active galactic nuclei (AGNs), but many questions remain unre…