Constraining the neutrino emission of gravitationally lensed Flat-Spectrum Radio Quasars with ANTARES data
arXiv:1407.8525 · doi:10.1088/1475-7516/2014/11/017
Abstract
This paper proposes to exploit gravitational lensing effects to improve the sensitivity of neutrino telescopes to the intrinsic neutrino emission of distant blazar populations. This strategy is illustrated with a search for cosmic neutrinos in the direction of four distant and gravitationally lensed Flat-Spectrum Radio Quasars. The magnification factor is estimated for each system assuming a singular isothermal profile for the lens. Based on data collected from 2007 to 2012 by the ANTARES neutrino telescope, the strongest constraint is obtained from the lensed quasar B0218+357, providing a limit on the total neutrino luminosity of this source of . This limit is about one order of magnitude lower than those previously obtained in the ANTARES standard point source searches with non-lensed Flat-Spectrum Radio Quasars.
12 pages, 1 figure, 1 table; abstract shortened and references added
References in corpus (8)
- Roma-BZCAT: A multifrequency catalogue of Blazars
- Relativistic Beaming and the Intrinsic Properties of Extragalactic Radio Jets
- Time-Integrated Searches for Point-like Sources of Neutrinos with the 40-String IceCube Detector
- Search for a diffuse flux of high-energy with the ANTARES neutrino telescope
- TANAMI Blazars in the IceCube PeV Neutrino Fields
- Gravitational lensing of transient neutrino sources by black holes
- Gravitational Lensing of Supernova Neutrinos
- Implications of the VHE Gamma-Ray Detection of the Quasar 3C279