activity
20092026
most citedThe Spectral Energy Distribution of Fermi bright blazars

1k citations · 2.1k across the 22 of their papers we have counts for

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13 papers · 1 filter

astro-ph.HE2026

Morphology-aware periodicity searches in Fermi-LAT blazars

Aaron A. Maldonado, Alberto Domínguez, Adithiya Dinesh +4

Standard periodicity searches in active galactic nuclei assume sinusoidal modulation, whereas gamma-ray blazar emission often features asymmetric flares and localized bursts. We in…

astro-ph.HE2026

Transient Relativistic Iron Emission Line from an X-ray Flaring Supermassive Black Hole

Xiurui Zhao, Marco Ajello, Francesca Civano +16

We report the discovery of the first transient relativistic iron Kα line in an Active Galactic Nucleus (AGN) J1047+5907. The line was detected 21.5 days (rest-frame) after an X-ray…

astro-ph.HE2025

Fast X-ray Variability from the Coronae of Supermassive Black Holes

Xiurui Zhao, Luca Comisso, Stefano Marchesi +4

We present the first systematic study of short-timescale X-ray variability in radio-quiet active galactic nuclei (AGN), utilizing archival Chandra observations of approximately 3,0…

astro-ph.HE2025

Unveiling Obscured Accretion in the Local Universe

Indrani Pal, Stefano Marchesi, Ross Silver +9

Heavily obscured Active Galactic Nuclei (AGN), especially Compton-thick sources with line-of-sight column density () 10 cm, are critical to underst…

astro-ph.HE2025

Contemporaneous X-ray and Optical Polarization of EHSP Blazar H 1426+428

Anuvab Banerjee, Akash Garg, Divya Rawat +17

We present the first contemporaneous X-ray and optical polarimetric measurement of the extremely high synchrotron peaked (EHSP) blazar H 1426+428. The X-ray polarimetric observatio…

astro-ph.HE2025

Distortions in Periodicity Analysis of Blazars: The Impact of Flares

Pablo Peñil, Nuria Torres-Albà, Alba Rico +3

Blazars, a unique class of active galactic nuclei, exhibit highly variable emission across the electromagnetic spectrum. This variability frequently manifests as intense flaring ev…

astro-ph.HE2018★ 37 cited

Unresolved Gamma-Ray Sky through its Angular Power Spectrum

M. Ackermann, M. Ajello, L. Baldini +107

The gamma-ray sky has been observed with unprecedented accuracy in the last decade by the Fermi large area telescope (LAT), allowing us to resolve and understand the high-energy Un…

astro-ph.HE2012★ 57 cited

Unidentifed gamma-ray sources: hunting gamma-ray blazars

F. Massaro, R. D'Abrusco, G. Tosti +2

One of the main scientific objectives of the ongoing Fermi mission is unveiling the nature of the unidentified gamma-ray sources (UGSs). Despite the large improvements of Fermi in…

astro-ph.HE2012★ 109 cited

Infrared Colors of the gamma-ray detected blazars

R. D'Abrusco, F. Massaro. M. Ajello, J. E. Grindlay +2

Blazars constitute the most enigmatic class of extragalactic gamma-ray sources, and their observational features have been ascribed to a relativistic jet closely aligned to the lin…

astro-ph.HE2012★ 172 cited

Identification of the infrared non-thermal emission in Blazars

F. Massaro, R. D'Abrusco, M. Ajello +2

Blazars constitute the most interesting and enigmatic class of extragalactic gamma-ray sources dominated by non-thermal emission. In this Letter, we show how the WISE infrared data…

astro-ph.HE2012★ 55 cited

Discovery of hard-spectrum γ-ray emission from the BL Lac object 1ES 0414+009

The HESS Collaboration, A. Abramowski, F. Acero +199

1ES 0414+009 (z = 0.287) is a distant high-frequency-peaked BL Lac object, and has long been considered a likely emitter of very-high energy (VHE, E>100 GeV) gamma-rays due to its…

astro-ph.HE2010★ 339 cited

Three years Swift-BAT Survey of AGN: reconciling theory and observations?

D. Burlon, M. Ajello, J. Greiner +4

It is well accepted that unabsorbed as well as absorbed AGN are needed to explain the nature and the shape of the Cosmic X-ray background, even if the fraction of highly absorbed o…

astro-ph.HE2010★ 23 cited

Swift-BAT Survey of Galactic Sources: Catalog and Properties of the populations

R. Voss, M. Ajello

We study the populations of X-ray sources in the Milky Way in the 15-55 keV band using a deep survey with the BAT instrument aboard the Swift observatory. We present the logN-logS…