Swift-XRT Observations and Upper Limits at Five LHAASO Galactic Sources
Abstract The detection of low-energy counterparts to gamma-ray sources is critical to understanding the nature of the astrophysical systems producing such high-energy emission. We report on Swift-XRT observations at five LHAASO gamma-ray sources with no known low-energy counterpart and scant previous X-ray observations. At four of the five LHAASO targets, we detect no significant X-ray point sources, while at 1LHAASO J1928+1813u we detect a single X-ray source that is likely related to X-ray emission from a local cool stellar system. These results suggest that many X-ray counterparts to LHAASO sources have X-ray flux below ≈10 −13 erg s −1 cm −2 , or have diffuse X-ray emission not visible in brief observations.
Authors
- S. Mujtaba Karim
- A. R. Walker
- Stephen DiKerby (ORCID: https://orcid.org/0000-0003-2633-2196)
- Ella Werre (ORCID: https://orcid.org/0009-0009-3820-4029)
Publication Details
- Journal
- Research Notes of the AAS
- Published
- 2025-04-17
- DOI
- https://doi.org/10.3847/2515-5172/adccb9
- Primary Topic
- Stellar, planetary, and galactic studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00