activity
20202026
most citedX-ray, UV and optical time delays in the bright Seyfert galaxy Ark 120 with co-ordinated Swift and ground-based observations

23 citations · 66 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2026

Detection of a triple nucleus in the Wolf-Rayet composite Sy 2 galaxy NGC 6764

Jochen Heidt, Francisco Pozo Nuñez, Nina Mackensen +2

We report adaptive-optics Ks-band imaging of the composite Seyfert 2 and Wolf-Rayet galaxy NGC 6764 (D = 32 Mpc), obtained with LUCI/SOUL at the Large Binocular Telescope. The nucl…

astro-ph.GA2026

Accretion-disk sizes in two quasars with interferometrically resolved broad-line regions at and

Francisco Pozo Nuñez, Eduardo Bañados, Swayamtrupta Panda +3

We present the first direct comparison between accretion-disk (AD) and broad-line region (BLR) sizes in quasars at z > 2, combining continuum reverberation mapping with interferome…

astro-ph.GA2026

A simulation-based quality-control framework for the broad-line region radius-luminosity relation

Juri Wladimir Seib, Francisco Pozo Nuñez, Sarah Elena Ivana Bosman

The broad-line region (BLR) radius-luminosity (R-L) relation underpins single-epoch black hole mass estimates in active galactic nuclei (AGN). The published Hβsample is heterogeneo…

astro-ph.GA2026

Adaptive optics imaging of the nuclei of Seyfert 2 galaxies: An unexpectedly high incidence of nuclear stellar rings

Nina Mackensen, Jochen Heidt, Francisco Pozo Nuñez

High-resolution imaging of active galactic nuclei (AGNs) on subkiloparsec scales is essential for investigating their fueling. Observations in the near-infrared (NIR) are especiall…

astro-ph.GA2026

HALO II: Constraining Hubble constant through continuum delay fitting of Fairall 9

Amit Kumar Mandal, Francisco Pozo Nuñez, Vikram Kumar Jaiswal +28

The Hubble tension remains one of the most significant unresolved problems in modern cosmology. A key question is whether it may arise from underestimated systematic uncertainties…

astro-ph.HE2026

Extraction method for response functions from X-ray light curves of AGN by optimization algorithm

Sanhanat Deesamutara, Tirawut Worrakitpoonpon, Poemwai Chainakun +4

We introduce a numerical optimization method to extract the X-ray reverberation response functions from the multi-band light curves of the active galactic nuclei. This approach doe…

astro-ph.GA2026

AGN Variability with Rubin Observatory in the 2030s

Swayamtrupta Panda, Francisco Pozo Nuñez, Hygor Benati Gonçalves +4

AGN variability offers a direct probe of accretion physics, disk structure, and black hole growth, but progress has been limited by sample size, cadence heterogeneity, and photomet…

astro-ph.GA2025

The evolution of obscured AGN across cosmic time -- A large quasar survey for the 2040s

Tanya Urrutia, Darshan Kakkad, Paula Sánchez-Sáez +21

We propose a large quasar demographic optical multi-object spectroscopic (MOS) survey targeting over 50 million AGN candidates up to the highest redshifts possible in the optical (…

astro-ph.GA2025★ 3 cited

HALO I: Photometric continuum reverberation mapping of Fairall 9

Amit Kumar Mandal, Francisco Pozo Nuñez, Vikram Kumar Jaiswal +23

We investigate the origin of inter-band continuum time delays in active galactic nuclei (AGNs) to study the structure and properties of their accretion disks. We aim to measure the…

astro-ph.GA2025

Kinematics and physical structure of Ou 5: A bipolar planetary nebula with extreme abundance discrepancy and an eclipsing binary core

William J. Henney, J. A. López, Ma. T. García-Díaz +5

We present new deep imaging and high-resolution spectroscopy of the extreme-abundance-discrepancy planetary nebula Ou 5, together with photoionization modelling aimed at probing it…

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★ 5 cited

Accretion disc reverberation mapping in a high-redshift quasar

F. Pozo Nuñez, E. Bañados, S. Panda +1

Powered by supermassive black holes at their centers, quasars are among the most luminous objects in the Universe, serving as important probes of cosmic history and galaxy evolutio…

astro-ph.GA2024★ 6 cited

Application of the FRADO model of BLR formation to the Seyfert galaxy NGC 5548 and the first step toward determining the Hubble constant

V. K. Jaiswal, Amit K. Mandal, R. Prince +5

The dynamical and geometric structures of the Broad Line Region (BLR), along with the origins of continuum time delays in active galaxies, remain topics of ongoing debate. In this…

astro-ph.GA2023★ 6 cited

Spectral variability studies in Active Galactic Nuclei: Exploring continuum and emission line regions in the age of LSST and JWST

Swayamtrupta Panda, Paola Marziani, Bozena Czerny +2

The investigation of emission line regions within active galaxies (AGNs) has a rich and extensive history, now extending to the use of AGNs and quasars as "standardizable" cosmolog…

astro-ph.HE2020★ 23 cited

X-ray, UV and optical time delays in the bright Seyfert galaxy Ark 120 with co-ordinated Swift and ground-based observations

A. P. Lobban, S. Zola, U. Pajdosz-Smierciak +17

We report on the results of a multiwavelength monitoring campaign of the bright, nearby Seyfert galaxy, Ark 120 using a ~50-day observing programme with Swift and a ~4-month co-ord…