activity
20222024
most citedNarrow line AGN selection in CEERS: spectroscopic selection, physical properties, X-ray and radio analysis

27 citations · 80 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2024★ 3 cited

A Multi-Wavelength Characterization of the Obscuring Medium at the Center of NGC 6300

D. Sengupta, N. Torres-Albà, A. Pizzetti +9

Most of the super-massive black holes in the Universe accrete material in an obscured phase. While it is commonly accepted that the "dusty torus" is responsible for the nuclear obs…

astro-ph.GA2024★ 7 cited

MAMBO -- An empirical galaxy and AGN mock catalogue for the exploitation of future surveys

X. López-López, M. Bolzonella, L. Pozzetti +13

Aims. We present MAMBO, a flexible and efficient workflow to build empirical galaxy and Active Galactic Nuclei (AGN) mock catalogues that reproduce the physical and observational p…

astro-ph.GA2024

An X-ray Significantly Variable, Luminous, Type 2 Quasar at z = 2.99 with a Massive Host Galaxy

Xiurui Zhao, Stefano Marchesi, Marco Ajello +8

We present a comprehensive X-ray analysis and spectral energy distribution (SED) fitting of WISEA J171419.96+602724.6, an extremely luminous type 2 quasar at = 2.99. The source…

astro-ph.GA2024★ 27 cited

Narrow line AGN selection in CEERS: spectroscopic selection, physical properties, X-ray and radio analysis

Giovanni Mazzolari, Jan Scholtz, Roberto Maiolino +11

In this work, we spectroscopically select narrow-line AGNs (NLAGNs) among the ~300 publicly available medium-resolution spectra of the Cosmic Evolution Early Release Science Survey…

astro-ph.GA2024★ 18 cited

A Cigale module tailored (not only) for Low-Luminosity AGN

I. E. López, G. Yang, G. Mountrichas +17

The spectral energy distribution (SED) of low-luminosity active galactic nuclei (LLAGN) presents challenges due to their faint emissions and the complexity of their accretion proce…

astro-ph.GA2024★ 3 cited

Ionised AGN outflows in the Goldfish galaxy -- The illuminating and interacting red quasar eFEDSJ091157.4+014327 at z 0.6

Blessing Musiimenta, Giovanna Speranza, Tanya Urrutia +12

Evolutionary models suggest that the initial growth phases of active galactic nuclei (AGN) are dust-enshrouded, and characterised by jet/wind outflows that should gradually clear t…

astro-ph.GA2023

Multi-phase characterization of AGN winds in 5 local type-2 quasars

G. Speranza, C. Ramos Almeida, J. A. Acosta-Pulido +9

We present MEGARA (Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía) Integral Field Unit (IFU) observations of 5 local type-2 quasars (QSO2s, z ) from the Qu…

astro-ph.GA2023

Obscuration beyond the nucleus: infrared quasars can be buried in extreme compact starbursts

Carolina Andonie, David M. Alexander, Claire Greenwell +14

In the standard quasar model, the accretion disk obscuration is due to the canonical dusty torus. Here, we argue that a substantial part of the quasar obscuration can come from the…

astro-ph.GA2023★ 20 cited

The miniJPAS survey: AGN & host galaxy co-evolution of X-ray selected sources

I. E. López, M. Brusa, S. Bonoli +35

Studies indicate strong evidence of a scaling relation in the local Universe between the supermassive black hole mass ($M_\rm{BH}$) and the stellar mass of their host galaxies ($M_…

astro-ph.IM2022

Web-based telluric correction made in Spain: spectral fitting of Vega-type telluric standards

D. de la Fuente, A. Marco, L. R. Patrick +7

Infrared spectroscopic observations from the ground must be corrected from telluric contamination to make them ready for scientific analyses. However, telluric correction is often…

astro-ph.HE2022★ 2 cited

Disentangling the nature of the prototype radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00 + 740511.2

E. J. Marchesini, V. Reynaldi, F. Vieyro +13

Context. The gamma-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT detection by crossmatching with Swift/XRT data. It has shown all the canonical…