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PreprintarXiv licencearXiv

The design and flight of the Payload for Ultrahigh Energy Observations (PUEO)

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60 listed; 73 in total.

Abstract

Sources of cosmic rays at ultrahigh energies (UHE, ≳ 1 EeV) are anticipated to give rise to neutrinos at similar energies by production via propagation interactions either within the source region or on cosmological scales. Measurements of the neutrino flux, flavor, and energy provide significant insight into those underlying processes governing UHE cosmic ray acceleration and propagation. Detecting neutrinos at these energies requires immense detector volumes due to their low predicted flux. We present the balloon-borne mission PUEO (Payload for Ultrahigh Energy Observations) which is an antenna array designed to detect the Askaryan emission from UHE neutrino interactions in the Antarctic ice. This paper reports on the design considerations and implementations for constructing PUEO, from the design parameters to the as-built validations.

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BibTeX
@misc{collaboration2026design,
  title = {{The design and flight of the Payload for Ultrahigh Energy Observations (PUEO)}},
  author = {PUEO Collaboration and Q. Abarr and S. Agarwal and J. Alfaro and S. Ali and P. Allison and J. Alvarez-Muñiz and T. Anderson and H. Barnett and A. Basharina-Freshville and J. J. Beatty and L. Beaufore and D. Z. Besson and M. Betts and R. Bose and D. Braun and B. Chamanbahar and P. Chen and Y. Chen and J. M. Clem and T. Coakley and A. Connolly and K. Couberly and L. Cremonesi and A. Cummings and P. Dasgupta and C. Deaconu and J. Flaherty and C. Godden and P. W. Gorham and C. Hornhuber and J. Hoffman and K. Hughes and A. Hynous and A. Jung and A. M. Kofman and Y. Ku and D. Kullgren and C. -Y. Kuo and P. Linton and L. Lisalda and T. C. Liu and W. Luszczak and S. C. Mackey and Z. Martin and K. McBride and C. Miki and J. Nam and D. A. Newmark and R. J. Nichol and A. Novikov and A. Nozdrina and E. Oberla and H. Pumphrey and D. Radomski and B. F. Rauch and R. Scrandis and D. Seckel and M. F. H. Seikh and J. Shiao},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.35675},
  eprint = {2610.35675},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.35675},
}
RIS
TY  - UNPB
TI  - The design and flight of the Payload for Ultrahigh Energy Observations (PUEO)
AU  - PUEO Collaboration
AU  - Q. Abarr
AU  - S. Agarwal
AU  - J. Alfaro
AU  - S. Ali
AU  - P. Allison
AU  - J. Alvarez-Muñiz
AU  - T. Anderson
AU  - H. Barnett
AU  - A. Basharina-Freshville
AU  - J. J. Beatty
AU  - L. Beaufore
AU  - D. Z. Besson
AU  - M. Betts
AU  - R. Bose
AU  - D. Braun
AU  - B. Chamanbahar
AU  - P. Chen
AU  - Y. Chen
AU  - J. M. Clem
AU  - T. Coakley
AU  - A. Connolly
AU  - K. Couberly
AU  - L. Cremonesi
AU  - A. Cummings
AU  - P. Dasgupta
AU  - C. Deaconu
AU  - J. Flaherty
AU  - C. Godden
AU  - P. W. Gorham
AU  - C. Hornhuber
AU  - J. Hoffman
AU  - K. Hughes
AU  - A. Hynous
AU  - A. Jung
AU  - A. M. Kofman
AU  - Y. Ku
AU  - D. Kullgren
AU  - C. -Y. Kuo
AU  - P. Linton
AU  - L. Lisalda
AU  - T. C. Liu
AU  - W. Luszczak
AU  - S. C. Mackey
AU  - Z. Martin
AU  - K. McBride
AU  - C. Miki
AU  - J. Nam
AU  - D. A. Newmark
AU  - R. J. Nichol
AU  - A. Novikov
AU  - A. Nozdrina
AU  - E. Oberla
AU  - H. Pumphrey
AU  - D. Radomski
AU  - B. F. Rauch
AU  - R. Scrandis
AU  - D. Seckel
AU  - M. F. H. Seikh
AU  - J. Shiao
PY  - 2026
DA  - 2026/10/26
PB  - arXiv
DO  - 10.48550/arxiv.2610.35675
UR  - https://arxiv.org/abs/2610.35675
AB  - Sources of cosmic rays at ultrahigh energies (UHE, ≳ 1 EeV) are anticipated to give rise to neutrinos at similar energies by production via propagation interactions either within the source region or on cosmological scales. Measurements of the neutrino flux, flavor, and energy provide significant insight into those underlying processes governing UHE cosmic ray acceleration and propagation. Detecting neutrinos at these energies requires immense detector volumes due to their low predicted flux. We present the balloon-borne mission PUEO (Payload for Ultrahigh Energy Observations) which is an antenna array designed to detect the Askaryan emission from UHE neutrino interactions in the Antarctic ice. This paper reports on the design considerations and implementations for constructing PUEO, from the design parameters to the as-built validations.
ER  -