activity
20182025
most citedThe remarkable X-ray variability of IRAS 13224-3809 I: The variability process

71 citations · 205 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2025

XMM/HST monitoring of the ultra-soft highly accreting Narrow Line Seyfert 1 RBS 1332

R. Middei, S. Barnier, F. G. Saturni +10

Ultra-soft narrow line Seyfert 1 (US-NLSy) are a poorly observed class of active galactic nuclei characterized by significant flux changes and an extreme soft X-ray excess. This pe…

astro-ph.HE2021★ 11 cited

Discovery of soft and hard X-ray time lags in low-mass AGNs

Labani Mallick, Daniel R. Wilkins, William N. Alston +5

The scaling relations between the black hole (BH) mass and soft lag properties for both active galactic nuclei (AGNs) and BH X-ray binaries (BHXRBs) suggest the same underlying phy…

astro-ph.HE2020★ 22 cited

The lively accretion disk in NGC 2992. I. Transient iron K emission lines in the high flux state

A. Marinucci, S. Bianchi, V. Braito +5

We report on one of the brightest flux levels of the Seyfert 2 galaxy NGC 2992 ever observed in X-rays, on May 2019. The source has been monitored every few days from March 26, 201…

astro-ph.HE2020★ 8 cited

X-raying winds in distant quasars: the first high-redshift wind duty cycle

E. Bertola, M. Dadina, M. Cappi +6

Theoretical models of wind-driven feedback from Active Galactic Nuclei (AGN) often identify Ultra-fast outflows (UFOs) as being the main cause for generating galaxy-size outflows,…

astro-ph.HE2019★ 52 cited

NuSTAR/XMM-Newton monitoring of the Seyfert 1 galaxy HE 1143-1810. Testing the two-corona scenario

F. Ursini, P. -O. Petrucci, S. Bianchi +11

We test the two-corona accretion scenario for active galactic nuclei in the case of the `bare' Seyfert 1 galaxy HE 1143-1810. We perform a detailed study of the broad-band UV--X-ra…

astro-ph.HE2019★ 11 cited

Multi-wavelength spectroscopy of the black hole candidate MAXI J1813-095 during its discovery outburst

M. Armas Padilla, T. Muñoz-Darias, J. Sánchez-Sierras +5

MAXI J1813-095 is an X-ray transient discovered during an outburst in 2018. We report on X-ray and optical observations obtained during this event, which indicate that the source i…