activity
20132026
most citedObservation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

1.2k citations · 3.1k across the 50 of their papers we have counts for

collaborators

51 papers

astro-ph.HE2026

Comment on "Fermi-LAT Galactic Center Excess Morphology of Dark Matter in Simulations of the Milky Way Galaxy"

Kevork N. Abazajian, Jason Kumar, Oscar Macias

Muru et al. [Phys. Rev. Lett. 135, 161005 (2025)] conclude from the HESTIA constrained simulations that the -ray morphologies of the Galactic Center Excess predicted by dark mat…

astro-ph.CO2026

Constraints on Annihilating Dark Matter from Gamma-Ray Background-Galaxy Shape Correlations: Model-independent Null Results and Moderate Template-based Signals

Masato Shirasaki, Deheng Song, Oscar Macias +2

We revisit the cross-correlation between the unresolved -ray background and galaxy shapes to constrain the annihilation cross section of particle dark matter. Our analysis uses…

astro-ph.HE2026

Geminga and Monogem in the CTAO Era: Probing TeV Halos and Cosmic-Ray Transport

Youyou Li, Oscar Macias, Manuela Vecchi +1

TeV halos around Geminga and Monogem (B0656+14) reveal regions of strongly suppressed diffusion near middle-aged pulsars. Determining the sizes and magnetic-field strengths of thes…

hep-ph2024★ 18 cited

Dark Matter Line Searches with the Cherenkov Telescope Array

S. Abe, J. Abhir, A. Abhishek +562

Monochromatic gamma-ray signals constitute a potential smoking gun signature for annihilating or decaying dark matter particles that could relatively easily be distinguished from a…

astro-ph.GA2024★ 17 cited

Robust inference of the Galactic centre gamma-ray excess spatial properties

Deheng Song, Christopher Eckner, Chris Gordon +6

The gamma-ray Fermi-LAT Galactic centre excess (GCE) has puzzled scientists for over 15 years. Despite ongoing debates about its properties, and especially its spatial distribution…

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

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★ 6 cited

TeV gamma-ray sensitivity to velocity-dependent dark matter models in the Galactic Center

Alessandro Montanari, Oscar Macias, Emmanuel Moulin

The center of the Milky Way is a prime site to search for signals of dark matter (DM) annihilation due to its proximity and expected high concentration of DM. The amplification of…

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…

hep-ex2023★ 1 cited

The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023)

GRAND Collaboration, Rafael Alves Batista, Aurélien Benoit-Lévy +96

The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses la…

astro-ph.HE2023★ 1 cited

Prospective Dark Matter Annihilation Signals From the Sagittarius Dwarf Spheroidal

Thomas A. A. Venville, Alan R. Duffy, Roland M. Crocker +2

The Sagittarius Dwarf Spheroidal galaxy (Sgr) is investigated as a target for DM annihilation searches utilising J-factor distributions calculated directly from a high-resolution h…

astro-ph.HE2022★ 22 cited

Gamma-ray emission from the Sagittarius Dwarf Spheroidal galaxy due to millisecond pulsars

Roland M. Crocker, Oscar Macias, Dougal Mackey +13

The Fermi Bubbles are giant, gamma-ray emitting lobes emanating from the nucleus of the Milky Way discovered in ~1-100 GeV data collected by the Large Area Telescope on board the F…

astro-ph.HE2022★ 10 cited

The Andromeda Gamma-Ray Excess: Background Systematics of the Millisecond Pulsars and Dark Matter Interpretations

Fabian Zimmer, Oscar Macias, Shin'ichiro Ando +2

Since the discovery of an excess in gamma rays in the direction of M31, its cause has been unclear. Published interpretations focus on a dark matter or stellar related origin. Stud…

astro-ph.HE2022

Assessing the Impact of Hydrogen Absorption on the Characteristics of the Galactic Center Excess

Martin Pohl, Oscar Macias, Phaedra Coleman +1

We present a new reconstruction of the distribution of atomic hydrogen in the inner Galaxy that is based on explicit radiation-transport modelling of line and continuum emission an…

hep-ph2022

Snowmass2021 Cosmic Frontier White Paper: Puzzling Excesses in Dark Matter Searches and How to Resolve Them

Rebecca K. Leane, Seodong Shin, Liang Yang +36

Intriguing signals with excesses over expected backgrounds have been observed in many astrophysical and terrestrial settings, which could potentially have a dark matter origin. Ast…

hep-ph2022★ 2 cited

Snowmass2021 Cosmic Frontier: Synergies between dark matter searches and multiwavelength/multimessenger astrophysics

Shin'ichiro Ando, Sebastian Baum, Michael Boylan-Kolchin +23

This whitepaper focuses on the astrophysical systematics which are encountered in dark matter searches. Oftentimes in indirect and also in direct dark matter searches, astrophysica…

astro-ph.HE2021

Measuring the smearing of the Galactic 511 keV signal: positron propagation or supernova kicks?

Thomas Siegert, Roland M. Crocker, Oscar Macias +4

We use 15 years of -ray data from INTEGRAL/SPI in a refined investigation of the morphology of the Galactic bulge positron annihilation signal. Our spatial analysis confirms tha…

astro-ph.CO2021

Dark matter constraints with stacked gamma rays scales with the number of galaxies

Daiki Hashimoto, Atsushi J. Nishizawa, Masahiro Takada +1

Low-surface-brightness galaxies (LSBGs) are interesting targets for searches of dark matter emission due to their low baryonic content. However, predicting their expected dark matt…

astro-ph.HE2021★ 46 cited

Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal

Anuj Gautam, Roland M. Crocker, Lilia Ferrario +4

Gamma-ray data from the Fermi-Large Area Telescope reveal an unexplained, apparently diffuse, signal from the Galactic bulge that peaks near 2 GeV with an approximately spherical i…

astro-ph.HE2021★ 18 cited

Cherenkov Telescope Array sensitivity to the putative millisecond pulsar population responsible for the Galactic center excess

Oscar Macias, Harm van Leijen, Deheng Song +3

The leading explanation of the Galactic center -ray excess is the extended emission from a unresolved population of millisecond pulsars (MSPs) in the Galactic b…

astro-ph.HE2021★ 28 cited

Evidence for a high-energy tail in the gamma-ray spectra of globular clusters

Deheng Song, Oscar Macias, Shunsaku Horiuchi +2

Millisecond pulsars are very likely the main source of gamma-ray emission from globular clusters. However, the relative contributions of two separate emission processes--curvature…

astro-ph.HE2020★ 32 cited

Comparing the Galactic Bulge and Galactic Disk Millisecond Pulsars

Harrison Ploeg, Chris Gordon, Roland Crocker +1

The Galactic Center Excess (GCE) is an extended gamma-ray source in the central region of the Galaxy found in Fermi Large Area Telescope (Fermi-LAT) data. One of the leading explan…

astro-ph.HE2020★ 71 cited

Prospects for Heavy WIMP Dark Matter with CTA: the Wino and Higgsino

Lucia Rinchiuso, Oscar Macias, Emmanuel Moulin +2

TeV-scale particles that couple to the standard model through the weak force represent a compelling class of dark matter candidates. The search for such Weakly Interacting Massive…

astro-ph.CO2020★ 109 cited

Green Bank and Effelsberg Radio Telescope Searches for Axion Dark Matter Conversion in Neutron Star Magnetospheres

Joshua W. Foster, Yonatan Kahn, Oscar Macias +6

Axion dark matter (DM) may convert to radio-frequency electromagnetic radiation in the strong magnetic fields around neutron stars. The radio signature of such a process would be a…