Pith. sign in

REVIEW

Energy dependence of Ti/Fe ratio in the Galactic cosmic rays measured by the ATIC-2 experiment

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 0905.0049 v1 pith:WHFVOVNH submitted 2009-05-01 astro-ph.HE

V.I. Zatsepin , A.D. Panov , N.V. Sokolskaya , J.H.Adams , Jr. , H.S. Ahn , G.L. Bashindzhagyan , J. Chang
show 11 more authors
M. Christl A.R. Fazely T.G. Guzik J.B. Isbert K.C. Kim E.N. Kouznetsov M.I. Panasyuk E.S. Seo J. Watts J.P. Wefel J. Wu
This is my paper · ORCID
classification astro-ph.HE
keywords energycosmicdependenceexperimentgalacticnucleonratiorays
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

Titanium is a rare, secondary nucleus among Galactic cosmic rays. Using the Silicon matrix in the ATIC experiment, Titanium has been separated. The energy dependence of the Ti to Fe flux ratio in the energy region from 5 GeV per nucleon to about 500 GeV per nucleon is presented.

Discussion (0). Continue with ORCID to comment.

Pith tools