EPJ Web Conf.
Volume 280, 2023RICAP-22, 8th Roma International Conference on Astroparticle Physics
|Number of page(s)||2|
|Published online||20 March 2023|
Tracking millisecond pulsars responsible for the Fermi GeV excess
LAPTh, CNRS, USMB,
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/).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.