The rate of cosmic ray showers at large zenith angles: a step towards the detection of ultra-high energy neutrinos by the Pierre Auger Observatory
- DOI
- 10.1016/s0927-6505(00)00114-6
- Published
- 2000-09
- Container
- Astroparticle Physics
- Publisher
- Elsevier BV
- Open access
- unknown
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Cite this work
BibTeX
@article{allodium:10.1016/s0927-6505-00-00114-6,
title = {The rate of cosmic ray showers at large zenith angles: a step towards the detection of ultra-high energy neutrinos by the Pierre Auger Observatory},
author = {M. Ave and R.A. Vázquez and E. Zas and J.A. Hinton and A.A. Watson},
year = {2000},
journal = {Astroparticle Physics},
doi = {10.1016/s0927-6505(00)00114-6},
url = {https://doi.org/10.1016/s0927-6505(00)00114-6}
}RIS
TY - JOUR TI - The rate of cosmic ray showers at large zenith angles: a step towards the detection of ultra-high energy neutrinos by the Pierre Auger Observatory AU - M. Ave AU - R.A. Vázquez AU - E. Zas AU - J.A. Hinton AU - A.A. Watson PY - 2000 JO - Astroparticle Physics DO - 10.1016/s0927-6505(00)00114-6 UR - https://doi.org/10.1016/s0927-6505(00)00114-6 ER -
APA
Ave, M., Vázquez, R., Zas, E., Hinton, J., & Watson, A. (2000). The rate of cosmic ray showers at large zenith angles: a step towards the detection of ultra-high energy neutrinos by the Pierre Auger Observatory. Astroparticle Physics. https://doi.org/10.1016/s0927-6505(00)00114-6
Source records
- crossref · retrieved 2026-09-26T04:03:11.287Z