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Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
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Testing the Sensitivity of the Galactic Center Excess to the Point Source Mask.
Yi-Ming Zhong1, Samuel D McDermott2, Ilias Cholis3
1Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA.
Physical Review Letters
|July 1, 2020
Summary
The Fermi Large Area Telescope
Area of Science:
- Astrophysics
- Gamma-ray astronomy
Background:
- The Galactic Center exhibits an excess of gamma rays in Fermi-LAT data.
- The Fermi Large Area Telescope (Fermi-LAT) has released an updated point source catalog (4FGL).
Purpose of the Study:
- To investigate the nature of the Galactic Center excess using the new 4FGL catalog.
- To assess the contribution of point sources to the observed gamma-ray excess.
Main Methods:
- Performed the first template fit utilizing a mask based on the 4FGL catalog.
- Searched for point sources and masked them out to analyze remaining emission.
Main Results:
- The gamma-ray excess at the Galactic Center persists even with the 4FGL catalog mask.
- Masking 4FGL point sources eliminates a sizable excess of bright pixels in the inner Galaxy.
- Identified bright sources lacking known counterparts.
Conclusions:
- Point sources have a restricted ability to account for the Galactic Center excess.
- Strong constraints are placed on point source luminosity functions that could explain the smooth emission.

