Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
arXiv:2512.23458 · doi:10.3847/1538-4365/ae58a1
Abstract
The DArk Matter Particle Explorer (DAMPE) is a space-borne high-energy particle detector that surveys the -ray sky above with a peak acceptance of . With the 102 months of data collected by DAMPE, we show that the Fermi bubbles are detected at a significance of and identify a GeV excess in the direction of Galactic center at confidence. Both spectra and morphology are consistent with those observed by Fermi-LAT and the GeV excess component can be interpreted by the dark matter annihilation with a mass of GeV and a velocity-averaged cross section of for the channel. Our results thus provide the first independent detection of these two intriguing diffuse gamma-ray sources besides Fermi-LAT.
24 pages, 18 figures and 6 tables, accepted for publication in ApJS
References in corpus (49)
- Array Programming with NumPy
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- The mass distribution and gravitational potential of the Milky Way
- Giant Gamma-ray Bubbles from Fermi-LAT: AGN Activity or Bipolar Galactic Wind?
- The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV
- Incremental Fermi Large Area Telescope Fourth Source Catalog
- The Parkes multibeam pulsar survey: VI. Discovery and timing of 142 pulsars and a Galactic population analysis
- Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons
- Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT
- Background model systematics for the Fermi GeV excess
- The Spectrum and Morphology of the Fermi Bubbles
- The DArk Matter Particle Explorer mission
- A Tale of Tails: Dark Matter Interpretations of the Fermi GeV Excess in Light of Background Model Systematics
- Measurement of the cosmic-ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
- The Fermi Bubbles: Giant, Multi-Billion-Year-Old Reservoirs of Galactic Center Cosmic Rays
- Inverse Compton Origin of the Hard X-Ray and Soft Gamma-Ray Emission from the Galactic Ridge
- Detection of large-scale X-ray bubbles in the Milky Way halo
- The Origin of the Extragalactic Gamma-Ray Background and Implications for Dark-Matter Annihilation
- Dark matter local density determination: recent observations and future prospects
- GeV excess in the Milky Way: The Role of Diffuse Galactic gamma ray Emission template
- Measurement of the cosmic ray helium energy spectrum from 70 GeV to 80 TeV with the DAMPE space mission
- A New Model For The Loop-I (The North Polar Spur) Region
- High-Energy Gamma Rays from the Milky Way: Three-Dimensional Spatial Models for the Cosmic-Ray and Radiation Field Densities in the Interstellar Medium
- The characteristics of the Galactic center excess measured with 11 years of Fermi-LAT data
- Fermi Bubbles Inflated by Winds Launched from the Hot Accretion Flow in Sgr A*
- Detection of spectral hardenings in cosmic-ray boron-to-carbon and boron-to-oxygen flux ratios with DAMPE
- Millisecond pulsar interpretation of the Galactic center gamma-ray excess
- Foreground Mismodeling and the Point Source Explanation of the Fermi Galactic Center Excess
- The on-orbit calibration of DArk Matter Particle Explorer
- The Return of the Templates: Revisiting the Galactic Center Excess with Multi-Messenger Observations
- Inert Higgs Dark Matter for CDF-II W-boson Mass and Detection Prospects
- Fermi and eRosita bubbles as relics of the past activity of the Galactic black hole
- MAGIC observations of the diffuse -ray emission in the vicinity of the Galactic Centre
- Structure Formation Models Weaken Limits on WIMP Dark Matter from Dwarf Spheroidal Galaxies
- Testing the millisecond pulsar scenario of the Galactic center gamma-ray excess with very high energy gamma-rays
- Improving constraints on the extended mass distribution in the Galactic Center with stellar orbits
- Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
- Search for gamma-ray spectral lines with the DArk Matter Particle Explorer
- Explaining the GeV antiproton/ray excesses and W-boson mass anomaly in an inert two Higgs doublet model
- The North Polar Spur and Aquila Rift
- A Phantom Menace: On the Morphology of the Galactic Center Excess
- Robust inference of the Galactic centre gamma-ray excess spatial properties
- Simulation study of performance of the Very Large Area gamma-ray Space Telescope
- Robustness of the Galactic Center Excess Morphology Against Masking
- Search for the gamma-ray spectral lines with the DAMPE and the Fermi-LAT observations
- Study of the Global Alignment for the DAMPE Detector
- Boresight Alignment of DArk Matter Particle Explorer
- PSF Calibration of DAMPE for gamma-ray Observations
- The calibrations of DAMPE -ray effective area