Pith. sign in

REVIEW

The Extreme Energy Events HECR array: status and perspectives

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1703.06358 v1 pith:ZLZ4UTBA submitted 2017-03-18 astro-ph.HE astro-ph.IM

The Extreme Energy Events HECR array: status and perspectives

I. Gnesi , M. Abbrescia , C. Avanzini , L. Baldini , R. Baldini Ferroli , G. Batignani , G. Bencivenni , E. Bossini
show 60 more authors
A. Chiavassa C. Cicalo L. Cifarelli F. Coccetti E. Coccia A. Corvaglia D. De Gruttola S. De Pasquale A. Di Giovanni M. D'Incecco M. Dreucci F.L. Fabbri E. Fattibene A. Ferraro V. Frolov P. Galeotti M. Garbini G. Gemme S. Grazzi C. Gustavino D. Hatzifotiadu F. Liciulli P. La Rocca A. Maggiora O. Maragoto Rodriguez G. Maron B. Martelli M.N. Mazziotta S. Miozzi R. Nania F. Noferini F. Nozzoli M. Panareo M.P. Panetta R. Paoletti W. Park L. Perasso F. Pilo G. Piragino F. Riggi G.C. Righini M. Rizzi G. Sartorelli E. Scapparone M. Schioppa A. Scribano M. Selvi S. Serci E. Siddi S. Squarcia L. Stori M. Taiuti G. Terreni O.B.Visnyei M.C. Vistoli L. Votano M.C.S. Williams S. Zani A. Zichichi R. Zuyeuski
This is my paper
classification astro-ph.HE astro-ph.IM
keywords energyarraycosmiceventsextremefluxhecrmuon
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

The Extreme Energy Events Project is a synchronous sparse array of 52 tracking detectors for studying High Energy Cosmic Rays (HECR) and Cosmic Rays-related phenomena. The observatory is also meant to address Long Distance Correlation (LDC) phenomena: the network is deployed over a broad area covering 10 degrees in latitude and 11 in longitude. An overview of a set of preliminary results is given, extending from the study of local muon flux dependance on solar activity to the investigation of the upward-going component of muon flux traversing the EEE stations; from the search for anisotropies at the sub-TeV scale to the hints for observations of km-scale Extensive Air Shower (EAS).

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.