Abstract
We report the analysis of the gamma-ray variability of NGC 1275-the radio galaxy at the center of the Perseus cluster. NGC 1275 has been observed continuously with the Fermi Large Area Telescope over the last nine years. We applied different time-domain analysis methods including Fourier, wavelets and Bayesian methods, in order to search for quasi-periodic oscillations in the gamma-ray emission. We found no evidence for periodicities of astrophysical origin.
Original language | English (US) |
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Pages (from-to) | 167-171 |
Number of pages | 5 |
Journal | Proceedings of the International Astronomical Union |
DOIs | |
State | Accepted/In press - 2020 |
Keywords
- galaxies: Active
- galaxies: Jets
- galaxies: Nuclei
- gamma rays: Observations
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science