Implications of the VHE Gamma-Ray Detection of the Quasar 3C279
Markus Boettcher (Ohio Univ.), Anita Reimer (Stanford Univ.), Alan P., Marscher (Boston Univ.)

TL;DR
The paper analyzes the spectral energy distribution of quasar 3C279 during its VHE gamma-ray detection, suggesting multi-zone models and considering both leptonic and hadronic emission mechanisms to explain the observations.
Contribution
It provides a detailed interpretation of the VHE gamma-ray emission from 3C279, ruling out simple one-zone models and exploring multi-zone leptonic and hadronic scenarios.
Findings
One-zone SSC model is inconsistent with observations.
Multi-zone models better explain the data.
Hadronic models require extreme jet power.
Abstract
The MAGIC collaboration recently reported the detection of the quasar 3C279 at > 100 GeV gamma-ray energies. Here we present simultaneous optical (BVRI) and X-ray (RXTE PCA) data from the day of the VHE detection and discuss the implications of the snap-shot spectral energy distribution for jet models of blazars. A one-zone synchrotron-self-Compton origin of the entire SED, including the VHE gamma-ray emission can be ruled out. The VHE emission could, in principle, be interpreted as Compton upscattering of external radiation (e.g., from the broad-line regions). However, such an interpretation would require either an unusually low magnetic field of B ~ 0.03 G or an unrealistically high Doppler factor of Gamma ~ 140. In addition, such a model fails to reproduce the observed X-ray flux. This as well as the lack of correlated variability in the optical with the VHE gamma-ray emission and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
