activity
20172026
most citedProbing the geometry and motion of AGN coronae through accretion disc emissivity profiles

65 citations · 287 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2026

Investigating the Periodic X-ray Behaviour in the Eclipsing AGN NGC 6814

T. O. Hodd, L. C. Gallo, A. G. Gonzalez +2

A 2016 XMM-Newton X-ray light curve of the Seyfert 1.5 galaxy NGC 6814 exhibited clear eclipsing behaviour, with distinct ingress and egress, during half of the observation. Here,…

astro-ph.HE2025

A Spectral Energy Distribution Variability Study of the Eclipsing AGN NGC 6814

L. K. Pothier-Bogoslowski, L. C. Gallo, A. G. Gonzalez +2

The local Seyfert 1.5 active galactic nucleus (AGN), NGC 6814, is known to exhibit complex variability, eclipses, and even changing-look behaviour. In this work, we utilize optical…

astro-ph.HE2023★ 9 cited

Applying wavelet analysis to the X-ray light curves of active galactic nuclei and quasi-periodic eruptions

Akshay Ghosh, L. C. Gallo, A. G. Gonzalez

In this work, we examine the application of the wavelet transform to the X-ray timing analyses of active galactic nuclei (AGN) and quasi-periodic eruption sources (QPEs). Several s…

astro-ph.HE2023★ 35 cited

Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios

S. Komossa, D. Grupe, A. Kraus +9

The project MOMO (Multiwavelength Observations and Modelling of OJ 287) was set up to test predictions of binary supermassive black hole (SMBH) scenarios and to understand disk-jet…

astro-ph.HE2023★ 26 cited

MOMO VI: Multifrequency radio variability of the blazar OJ 287 from 2015-2022, absence of predicted 2021 precursor-flare activity, and a new binary interpretation of the 2016/2017 outburst

S. Komossa, A. Kraus, D. Grupe +12

Based on our dedicated Swift monitoring program, MOMO, OJ 287 is one of the best-monitored blazars in the X-ray--UV--optical regime. Here, we report results from our accompanying,…

astro-ph.HE2023★ 8 cited

The Collisional and Photoionized Plasma in the Polarized NLS1 galaxy Mrk 1239

Margaret Z. Buhariwalla, Luigi C. Gallo, J. Mao +4

Mrk 1239 is a highly polarized NLS1 in the optical band, whose keV spectrum has remained remarkably consistent over more than two decades of observation. Previous analysis…