activity
20112026
most citedBackground model systematics for the Fermi GeV excess

466 citations · 3.1k across the 85 of their papers we have counts for

collaborators

88 papers

astro-ph.CO2026

MeV dark matter decay forecasts for the COSI mission

Robin Anthony-Petersen, Orion Ning, Yu Watanabe +21

The decay of dark matter (DM) is a generic prediction of many particle physics models, producing distinctive monochromatic signatures in environments such as the Galactic halo. Sea…

astro-ph.GA2026

Stellar flares cannot explain the Galactic 511 keV emission

Saurabh Mittal, Thomas Siegert, Francesca Calore +12

The origin of the 511 keV line signal in the Milky Way remains unresolved despite decades of observations. The measured flux of $\sim 3 \times 10^{-3}\,\mathrm{ph\,cm^{-2}\,s^{-1}}…

hep-ph2026

The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles

Ariel Arza, Deniz Aybas, Shyam Balaji +124

Axions and other very weakly interacting slim particles (WISPs), with masses below 1 GeV, arise naturally in many extensions of the Standard Model of particle physics. In particula…

astro-ph.HE2026

-Ray Lines -- Signatures of Nucleosynthesis, Cosmic Rays, Positron Annihilation, and Fundamental Physics

Thomas Siegert, Francesca Calore, Pierre Jean +6

The nuclear -ray lines in the MeV range of the electromagnetic spectrum hold a vast variety of astrophysical, particle-physical, and fundamental physical information that is oth…

astro-ph.HE2025

Search for Axion-Like Particles from Nearby Pre-Supernova Stars

Saurabh Mittal, Thomas Siegert, Francesca Calore +7

Axion-like particles (ALPs) are hypothetical pseudoscalar bosons that arise in many extensions of the Standard Model and are well-motivated dark matter candidates. Nearby massive s…

astro-ph.HE2025★ 1 cited

Multiwavelength identification of millisecond pulsar candidates in the Galactic bulge

J. Berteaud, F. Calore, M. Clavel +4

The existence of a population of millisecond pulsars in the Galactic bulge is supported, along with other evidence, by the Fermi GeV excess, an anomalous γ-ray emission detected al…

hep-ph2025

Low-frequency radio telescopes sensitivity to light dark matter

Ruben Zatini, Francesca Calore, Pasquale Dario Serpico

Ground-based radio telescopes are routinely used to search for light dark matter (DM) candidates such as axion-like particles or dark photons. These instruments face however inhere…

hep-ph2025

Stellar-like Galactic center excess challenges particle dark matter

Silvia Manconi, Christopher Eckner, Francesca Calore +1

The Galactic Center (GC) is potentially hosting the largest indirect signal from particle dark matter (DM), which in many well-motivated models would produce gamma rays as their fi…

hep-ph2025★ 1 cited

Cosmic-ray cooling by dark matter in astrophysical jets

Dimitrios Kantzas, Francesca Calore, Marco Chianese

Astrophysical jets from powerful active galactic nuclei (AGN) have recently been proposed as promising probes of dark matter (DM) in the sub-GeV mass range. AGN launch relativistic…

astro-ph.HE2025★ 1 cited

Lecture Notes: WISPs in gamma-ray astrophysics

Francesca Calore, Christopher Eckner

These lecture notes provide an overview of high-energy astrophysical processes involving axions, axion-like particles (ALPs), and other weakly interacting slim particles (WISPs) fo…

astro-ph.HE2025

A robust neural determination of the source-count distribution of the Fermi-LAT sky at high latitudes

Christopher Eckner, Noemi Anau Montel, Florian List +2

Over the past 16 years, the Fermi Large Area Telescope (LAT) has significantly advanced our view of the GeV gamma-ray sky, yet several key questions remain - such as the compositio…

hep-ph2025

Can local White Dwarfs constrain Dark Matter interactions?

Pooja Bhattacharjee, Sandra Robles, Stephan A. Meighen-Berger +1

We investigate whether nearby white dwarfs (WDs) can constrain dark matter (DM) interactions with ordinary matter. As experimental sensitivity improves, driven by the Gaia mission,…

astro-ph.HE2025

Discovery of 15 new pulsars at high Galactic Latitudes with FAST

Xin Xu, Shi Dai, Qijun Zhi +9

We present the discovery and timing results of 15 pulsars discovered in a high Galactic latitude survey conducted with the Five-hundred-meter Aperture Spherical Telescope (FAST). T…

astro-ph.HE2025

Detecting dark matter sub-halos in the Galactic plane with the Cherenkov Telescope Array Observatory

Christopher Eckner, Veronika Vodeb, Tejas Satheesh +4

Numerous observations confirm the existence of dark matter (DM) at astrophysical and cosmological scales. Theory and simulations of galaxy formation predict that DM should cluster…

astro-ph.HE2024

No evidence for gamma-ray emission from the Sagittarius dwarf spheroidal galaxy

Christopher Eckner, Silvia Manconi, Francesca Calore

More than a decade ago, the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope unveiled the existence of two gigantic gamma-ray lobes known as the Fermi bubbles. While…

astro-ph.GA2024★ 14 cited

New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing

Andrés Bañares-Hernández, Francesca Calore, Jorge Martin Camalich +1

We perform a combined analysis of stellar kinematics and line-of-sight accelerations of millisecond pulsars to investigate the mass contents of Omega Centauri. We consider multiple…

astro-ph.HE2024★ 3 cited

Quiescent black hole X-ray binaries as multi-messenger sources

Dimitrios Kantzas, Francesca Calore

The origin of Galactic cosmic rays (CRs) is unknown even though they have traditionally been connected to supernovae based on energetic arguments. In the past decades, Galactic bla…

astro-ph.HE2024

An Image-Based Search for Pulsar Candidates in the MeerKAT Bulge Survey

Dale A. Frail, Emil Polisensky, Scott D. Hyman +13

We report on the results of an image-based search for pulsar candidates toward the Galactic bulge. We used mosaic images from the MeerKAT radio telescope, that were taken as part o…

hep-ph2024★ 7 cited

Constraining gravitational-wave backgrounds from conversions into photons in the Galactic magnetic field

Alessandro Lella, Francesca Calore, Pierluca Carenza +1

High-frequency gravitational waves ( MHz) may provide a unique signature for the existence of exotic physics. The lack of current and future gravitational-wave experim…

astro-ph.HE2024★ 1 cited

Simulation-based inference of radio millisecond pulsars in globular clusters

Joanna Berteaud, Christopher Eckner, Francesca Calore +2

Millisecond pulsars (MSPs) are abundant in globular clusters (GCs), which offer favorable environments for their creation. While the advent of recent, powerful facilities led to a…

hep-ph2024★ 14 cited

Probing protoneutron stars with gamma-ray axionscopes

Alessandro Lella, Francesca Calore, Pierluca Carenza +4

Axion-like particles (ALPs) coupled to nucleons can be efficiently produced in the interior of protoneutron stars (PNS) during supernova (SN) explosions. If these ALPs are also cou…

astro-ph.HE2024

A targeted radio pulsar survey of redback candidates with MeerKAT

T. Thongmeearkom, C. J. Clark, R. P. Breton +18

Redbacks are millisecond pulsar binaries with low mass, irradiated companions. These systems have a rich phenomenology that can be used to probe binary evolution models, pulsar win…

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.HE2024

The Galactic center excess at the highest energies: morphology and photon-count statistics

Silvia Manconi, Francesca Calore, Fiorenza Donato

The nature of the GeV gamma-ray Galactic center excess (GCE) in the data of Fermi-Large Area Telescope (LAT) is still to be unveiled. We present a new analysis of the inner Galaxy…