| Issue |
A&A
Volume 707, March 2026
|
|
|---|---|---|
| Article Number | A61 | |
| Number of page(s) | 6 | |
| Section | Numerical methods and codes | |
| DOI | https://doi.org/10.1051/0004-6361/202556902 | |
| Published online | 03 March 2026 | |
A catalog of gamma-ray source candidates from 16 years of Fermi-LAT data at |b| > 10°
Department of Physics, K. N. Toosi University of Technology,
PO Box 15875-4416,
Tehran,
Iran
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
19
August
2025
Accepted:
29
December
2025
Abstract
Context. Sixteen years of continuous observations with the Fermi Large Area Telescope (LAT) provide an unprecedented opportunity to search for faint or previously unrecognized γ-ray emitters, particularly at high energies where the angular resolution improves and the diffuse background is reduced.
Aims. We present a new catalog of γ-ray source candidates identified using a data-driven, clustering-based analysis of Pass 8 LAT data above 3 GeV at Galactic latitudes of |b| > 10°.
Methods. The pipeline integrates the SIeving MEthod for FInding Core, version 3 (SIMEFIC III), for photon denoising with the density-based spatial clustering of applications with noise (DBSCAN) algorithm.
Results. We detect 3112 γ-ray cluster candidates, of which 2932 are associated with known γ-ray sources. Crossmatching yields 37 counterparts in 1CGH, 23 in CRATES, 21 in Roma-BZCAT, and 17 in MST-12yr. The remaining 370 clusters have no known γ-ray counterpart and are proposed as new source candidates.
Key words: methods: data analysis / methods: numerical / methods: statistical / catalogs
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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