A spectral hardening in the Fermi-LAT Data of 1ES 0502+675

Author:

Zeng Yuhang12,Yan Dahai1ORCID,Hu Wen3ORCID,Wang Jiancheng1

Affiliation:

1. Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Observatories, Chinese Academy of Sciences , Kunming 650011, People’s Republic of China

2. School of Astronomy and Space Science, University of Chinese Academy of Sciences , Beijing 100049, People’s Republic of China

3. Department of Physics, Jinggangshan University , Jiangxi Province, Ji’an 343009, People’s Republic of China

Abstract

ABSTRACT The γ-ray spectral feature of the blazar 1ES 0502+675 is investigated by using Fermi Large Area Telescope Pass 8 data (between 100 MeV and 300 GeV) covering from 2008 August to 2021 April. A significant (∼4σ) hardening at ∼1 GeV is found in the γ-ray spectrum during a moderately flaring state (MJD 55050–55350). The photon index below and above the break energy is Γ1 = 2.36 ± 0.31 and Γ2 = 1.33 ± 0.11, respectively. In the rest of the observations, the γ-ray spectrum can be described by a power-law form with the photon index of ≈1.6. In the frame of a one-zone synchrotron self-Compton (SSC) model, the spectral hardening is interpreted as the transition between the synchrotron component and the SSC component. This could be the result of a slight increase of the break or maximum Lorentz factor of the electrons.

Funder

NASA

National Natural Science Foundation of China

CAS

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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