Discovery of High-energy and Very High Energy Gamma-ray Emission from the Blazar RBS 0413
VERITAS Collaboration: E. Aliu, S. Archambault, T. Arlen, T. Aune, M., Beilicke, W. Benbow, M. Boettcher, A. Bouvier, S. M. Bradbury, J. H. Buckley,, V. Bugaev, K. Byrum, A. Cannon, A. Cesarini, L. Ciupik, E. Collins-Hughes, M., P. Connolly, P. Coppi, W. Cui, G. Decerprit

TL;DR
This paper reports the first detection of high-energy and very high-energy gamma-ray emission from the blazar RBS 0413, combining observations from VERITAS and Fermi-LAT, and discusses spectral modeling with different emission scenarios.
Contribution
It presents the discovery of gamma-ray emission from RBS 0413 with detailed spectral analysis and modeling, highlighting the preference for complex emission models over simple ones.
Findings
VHE gamma-ray emission detected with 5.5 sigma significance
HE gamma-ray emission detected with over 9 sigma significance
Spectral energy distribution modeling favors combined emission models
Abstract
We report on the discovery of high-energy (HE; E > 0.1 GeV) and very high-energy (VHE; E > 100 GeV) gamma-ray emission from the high-frequency-peaked BL Lac object RBS 0413. VERITAS, a ground-based gamma-ray observatory, detected VHE gamma rays from RBS 0413 with a statistical significance of 5.5 standard deviations (sigma) and a gamma-ray flux of (1.5 \pm 0.6stat \pm 0.7syst) \times 10^(-8) photons m^(-2) s^(-1) (\sim 1% of the Crab Nebula flux) above 250 GeV. The observed spectrum can be described by a power law with a photon index of 3.18 \pm 0.68stat \pm 0.30syst. Contemporaneous observations with the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope detected HE gamma rays from RBS 0413 with a statistical significance of more than 9 sigma, a power-law photon index of 1.57 \pm 0.12stat +0.11sys -0.12sys and a gamma-ray flux between 300 MeV and 300 GeV of (1.64 \pm…
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