WHY HAVE MANY OF THE BRIGHTEST RADIO-LOUD BLAZARS NOT BEEN DETECTED IN GAMMA-RAYS BY FERMI ?

Author:

Lister M. L.ORCID,Aller M. F.ORCID,Aller H. D.,Hovatta T.,Max-Moerbeck W.,Readhead A. C. S.,Richards J. L.ORCID,Ros E.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 45 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. A Comprehensive Study on the Mid-Infrared Variability of Blazars;Universe;2024-09-07

2. On the Origin of the X-Ray Emission in Heavily Obscured Compact Radio Sources;The Astrophysical Journal;2024-05-01

3. A Kpc-scale radio polarization study of PG BL Lacs with the uGMRT;Monthly Notices of the Royal Astronomical Society;2023-10-17

4. Multiple imaging of the quasar 2005 + 403 formed by anisotropic scattering;Monthly Notices of the Royal Astronomical Society;2023-10-06

5. Characterizing the Emission Region Properties of Blazars;The Astrophysical Journal Supplement Series;2023-09-01

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