Evidence for Unresolved γ-Ray Point Sources in the Inner Galaxy
We present a new method to characterize unresolved point sources (PSs) generalizing traditional template fits to account for non-Poissonian photon statistics. We apply this method to Fermi Large Area Telescope γ-ray data to characterize PS populations at high latitudes and in the Inner Galaxy. We fi...
| Main Authors: | , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
American Physical Society
2016
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| Online Access: | http://hdl.handle.net/1721.1/101116 https://orcid.org/0000-0001-9531-1319 https://orcid.org/0000-0002-6809-7545 https://orcid.org/0000-0001-9699-9047 |