4.6 Article

Search for muon neutrinos from gamma-ray bursts with the ANTARES neutrino telescope using 2008 to 2011 data

Journal

ASTRONOMY & ASTROPHYSICS
Volume 559, Issue -, Pages -

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201322169

Keywords

neutrinos; gamma-ray burst: general; methods: numerical

Funding

  1. Centre National de la Recherche Scientifique (CNRS)
  2. Commissariat a l'energie atomique et aux energies alternatives (CEA)
  3. Agence National de la Recherche (ANR)
  4. Commission Europeenne (FEDER fund)
  5. Commission Europeenne (Marie Curie Program)
  6. Region Alsace (contrat CPER)
  7. Region Provence-Alpes-Cete d'Azur
  8. Departement du Var and Ville de La Seyne-sur-Mer, France
  9. Bundesministerium fur Bildung und Forschung (BMBF), Germany
  10. Istituto Nazionale di Fisica Nucleare (INFN), Italy
  11. Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands
  12. Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia
  13. National Authority for Scientific Research (ANCS), Romania
  14. Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain
  15. Agence de l'Oriental and CNRST, Morocco

Ask authors/readers for more resources

Aims. We search for muon neutrinos in coincidence with GRBs with the ANTARES neutrino detector using data from the end of 2007 to 2011. Methods. Expected neutrino fluxes were calculated for each burst individually. The most recent numerical calculations of the spectra using the NeuCosmA code were employed, which include Monte Carlo simulations of the full underlying photohadronic interaction processes. The discovery probability for a selection of 296 GRBs in the given period was optimised using an extended maximum-likelihood strategy. Results. No significant excess over background is found in the data, and 90% confidence level upper limits are placed on the total expected flux according to the model.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.6
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available