| Issue |
EPJ Web Conf.
Volume 280, 2023
RICAP-22, 8th Roma International Conference on Astroparticle Physics
|
|
|---|---|---|
| Article Number | 09003 | |
| Number of page(s) | 2 | |
| Section | Poster | |
| DOI | https://doi.org/10.1051/epjconf/202328009003 | |
| Published online | 20 March 2023 | |
https://doi.org/10.1051/epjconf/202328009003
Tracking millisecond pulsars responsible for the Fermi GeV excess
1
LAPTh, CNRS, USMB,
F-74940
Annecy, France
2
Univ. Grenoble Alpes, CNRS, IPAG,
F-38000
Grenoble, France
* e-mail: μberteaud@lapth.cnrs.fr
Published online: 20 March 2023
More than 10 years ago, an excess of γ-ray photons coming from the Galactic center was discovered in the Fermi-LAT data. First attributed to dark matter, it has since been shown that it should have at least a partial stellar origin. One hypothesis is the presence of a population of millisecond pulsars (MSPs) confined in the Galactic bulge. We here present our recent progress in the selection of MSP candidates.
© The Authors, published by EDP Sciences, 2023
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
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