activity
20092026
most citedScience with the Cherenkov Telescope Array

241 citations · 1.1k across the 63 of their papers we have counts for

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Showing astro-ph.HEShow all

35 papers · 1 filter

astro-ph.HE2023

Chasing Gravitational Waves with the Cherenkov Telescope Array

Jarred Gershon Green, Alessandro Carosi, Lara Nava +563

The detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts…

astro-ph.HE2023★ 3 cited

Joint searches by FACT, H.E.S.S., MAGIC and VERITAS for VHE gamma-ray emission associated with neutrinos detected by IceCube

Fabian Schüssler, Halim Ashkar, Elisa Bernardini +11

The sources of the astrophysical flux of high-energy neutrinos detected by IceCube are still largely unknown, but searches for temporal and spatial correlation between neutrinos an…

astro-ph.HE2023

Variability studies of active galactic nuclei from the long-term monitoring program with the Cherenkov Telescope Array

Guillaume Grolleron, Josefa Becerra González, Jonathan Biteau +13

Blazars are active galactic nuclei (AGN) with a relativistic jet oriented toward the observer. This jet is composed of accelerated particles which can display emission over the ent…

astro-ph.HE2023

Dark matter searches in dwarf spheroidal galaxies with the Cherenkov Telescope Array

Francesco Gabriele Saturni, Michele Doro, Aldo Morselli +1

Dark matter (DM) is one of the major components in the Universe. However, at present its existence is still only inferred through indirect astronomical observations. DM particles c…

astro-ph.HE2023

Modelling of highly extended Gamma-ray emission around the Geminga Pulsar as detected with H.E.S.S

A. M. W. Mitchell, S. Caroff

Geminga is an enigmatic radio-quiet gamma-ray pulsar located at a mere 250 pc distance from Earth. Extended very-high-energy gamma-ray emission around the pulsar has been detected…

astro-ph.HE2021★ 3 cited

Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events

O. Sergijenko, A. Brown, D. Fiorillo +6

We investigate the possibility of detection of the VHE gamma-ray counterparts to the neutrino astrophysical sources within the Neutrino Target of Opportunity (NToO) program of CTA…

astro-ph.HE2021★ 4 cited

Photohadronic Modelling of the 2010 Gamma-ray Flare from Mrk 421

A. Rosales de León, A. M. Brown, P. M. Chadwick

Blazars are a subclass of active galactic nuclei (AGN) that have a relativistic jet with a small viewing angle towards the observer. Recent results based on hadronic scenarios have…

astro-ph.HE2020★ 28 cited

Locating the gamma-ray emission region in the brightest Fermi-LAT Flat Spectrum Radio Quasars

Atreya Acharyya, Paula M. Chadwick, Anthony M. Brown

We present a temporal and spectral analysis of the gamma-ray flux from nine of the brightest flat spectrum radio quasars (FSRQs) detected with the Fermi Large Area Telescope (LAT)…

astro-ph.HE2020★ 15 cited

A search for Centaurus A-like features in the spectra of Fermi-LAT detected radio galaxies

Cameron B. Rulten, Anthony M. Brown, Paula M. Chadwick

Motivated by the detection of a hardening in the gamma-ray spectrum of the radio galaxy Centaurus A, we have analysed ~10 years of Fermi-LAT observations of 26 radio galaxies to se…

astro-ph.HE2020★ 13 cited

Axion Constraints from Quiescent Soft Gamma-ray Emission from Magnetars

Sheridan J. Lloyd, Paula M. Chadwick, Anthony M. Brown +2

Axion-like-particles (ALPs) emitted from the core of a magnetar can convert to photons in its magnetosphere. The resulting photon flux is sensitive to the product of the ALP-…

astro-ph.HE2019★ 4 cited

Reply to a comment on `Understanding the gamma-ray emission from the globular cluster 47 Tuc: evidence for dark matter?'

Anthony M. Brown, Thomas Lacroix, Sheridan Lloyd +2

Analysing 9 years of Fermi-LAT observations, we recently studied the spectral properties of the prominent globular cluster 47 Tuc (Brown et al. 2018). In particular, we investigate…

astro-ph.HE2019★ 12 cited

Constraining Axion Mass through Gamma-ray Observations of Pulsars

Sheridan J. Lloyd, Paula M. Chadwick, Anthony M. Brown

We analyze 9 years of PASS 8 -LAT data in the 60500 MeV range and determine flux upper limits (UL) for 17 gamma-ray dark pulsars as a probe of axions produced by…

astro-ph.HE2019★ 8 cited

The glow of annihilating dark matter in Omega Centauri

Anthony M. Brown, Richard Massey, Thomas Lacroix +3

Dark matter (DM) is the most abundant material in the Universe, but has so far been detected only via its gravitational effects. Several theories suggest that pairs of DM particles…

astro-ph.HE2019★ 10 cited

Fermi-LAT Observations of Extreme Spectral Variability in IC 310

Jamie Graham, Anthony Brown, Paula Chadwick

We investigate the physical mechanisms of high-energy gamma-ray emission from the TeV-emitting misaligned active galactic nucleus IC 310. Eight years of data from the Fermi Large A…

astro-ph.HE2019★ 21 cited

Gamma-rays from SS433: evidence for periodicity

Kajwan Rasul, Paula M. Chadwick, Jamie A. Graham +1

In this paper we present our study of the gamma-ray emission from the microquasar SS433. Integrating over 9 years of Fermi-LAT \textsc{pass8} data, we detect SS433 with a significa…

astro-ph.HE2018★ 11 cited

Gamma-ray emission from high Galactic latitude globular clusters

Sheridan J. Lloyd, Paula M. Chadwick, Anthony M. Brown

We analyse 8 years of PASS 8 Fermi-LAT data, in the 60 MeV - 300 GeV energy range, from 30 high Galactic latitude globular clusters. Six of these globular clusters are detected wit…

astro-ph.HE2018★ 30 cited

Understanding the -ray emission from the globular cluster 47 Tuc: evidence for dark matter?

Anthony M. Brown, Thomas Lacroix, Sheridan Lloyd +2

47 Tuc was the first globular cluster observed to be -ray bright, with the -rays being attributed to a population of unresolved millisecond pulsars (MSPs). Recent kinematic d…

astro-ph.HE2017★ 8 cited

Fermi-LAT high AGN and the Extragalactic Background Light

Thomas Armstrong, Anthony M. Brown, Paula M. Chadwick

Observations of distant gamma-ray sources are hindered by the presence of the extragalactic background light (EBL). In order to understand the physical processes that result in the…

astro-ph.HE2016★ 13 cited

Gamma-ray Novae: Rare or Nearby?

Paul J. Morris, Garret Cotter, Anthony M. Brown +1

Classical Novae were revealed as a surprise source of gamma-rays in Fermi LAT observations. During the first 8 years since the LAT was launched, 6 novae in total have been detected…

astro-ph.HE2016★ 30 cited

Discovery of a new extragalactic source population of energetic particles

Anthony M. Brown, Celine Bœhm, Jamie Graham +3

We report the discovery of a statistically significant hardening in the Fermi-LAT -ray spectrum of Centaurus A's core, with the spectral index hardening from $Γ_{1}=2.73 \pm 0.0…

astro-ph.HE2016★ 26 cited

Localising the gamma-ray emission region during the June 2014 outburst of 3C 454.3

Rosemary T. Coogan, Anthony M. Brown, Paula M. Chadwick

In May - July 2014, the flat spectrum radio quasar 3C 454.3 exhibited strong flaring behaviour. Observations with the Large Area Telescope detector on-board the Fermi Gamma-ray Spa…

astro-ph.HE2015★ 79 cited

Search for Dark Matter Annihilation in the Galactic Center with IceCube-79

IceCube Collaboration, M. G. Aartsen, K. Abraham +310

The Milky Way is expected to be embedded in a halo of dark matter particles, with the highest density in the central region, and decreasing density with the halo-centric radius. Da…

astro-ph.HE2015★ 7 cited

The Detection of Fermi AGN above 100 GeV using Clustering Analysis

Thomas Armstrong, Anthony M. Brown, Paula M. Chadwick +1

The density-based clustering algorithm DBSCAN has been applied to the Fermi Large Area Telescope (LAT) dataset of GeV events with ,…

astro-ph.HE2015★ 15 cited

-ray observations of extraterrestrial neutrino track event positions

Anthony M. Brown, Jenni Adams, Paula M. Chadwick

In this paper we report the results of a -ray study of IceCube's extraterrestrial neutrino candidates detected as track-like events. Using 70 months of Fermi-LAT observations, a…