Robustness of the Galactic Center excess morphology against masking-Reference-Cited by-同舟云学术

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Robustness of the Galactic Center excess morphology against masking

Published:2024-06-11 Issue:12 Volume:109 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Zhong Yi-Ming¹²^ORCID,Cholis Ilias³

Affiliation:

1. City University of Hong Kong

2. University of Chicago

3. Oakland University

Funder

Aspen Center for Physics

National Science Foundation

Kavli Institute for Cosmological Physics, University of Chicago

Kavli Foundation

U.S. Department of Energy

Office of Science

High Energy Physics

New High Energy Physics Center at Rutgers University

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.109.123017/fulltext

Reference55 articles.

1. Dark matter annihilation in the Galactic Center as seen by the Fermi Gamma Ray Space Telescope

2. The consistency of Fermi-LAT observations of the galactic center with a millisecond pulsar population in the central stellar cluster

3. Origin of the gamma rays from the Galactic Center

4. Two emission mechanisms in the Fermi Bubbles: A possible signal of annihilating dark matter

5. Dark matter and pulsar model constraints from Galactic Center Fermi-LAT gamma-ray observations

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Applying simulation-based inference to spectral and spatial information from the Galactic Center gamma-ray excess;Journal of Cosmology and Astroparticle Physics;2024-07-01

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