Pith. sign in

REVIEW

Explanation to the article "On the calibration of ultra-high energy EASs at the Yakutsk array and Telescope Array"

Not yet reviewed by Pith; the record is open.

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 2410.01851 v1 pith:XZFV27OI submitted 2024-10-01 astro-ph.HE astro-ph.IM

classification astro-ph.HEastro-ph.IM
keywords energyarrayarxivastro-phcalibrationdepositestimationformula
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We provide a detailed commentary on the energy calibration of the TA experiment described in our paper (arXiv:2404.16948 [astro-ph.HE]). That paper concludes that the TA energy estimation, which is tied to optical measurements, might be incorrect. A response from members of the TA Collaboration (arXiv:2407.12892 [astro-ph.HE]) states that this conclusion is wrong and "stems from a misinterpretation and an incorrect application of the TA energy deposit formula". Here we demonstrate that our formula for energy deposit is not in fact a rescaled modification of the TA equation, but follows from description of the processes occurring during the passage of charged particles through 1.2 cm thick scintillator. Our estimation of the TA detector response implies the correctness of the cosmic ray spectrum derived from readings of surface detectors of the array.

Discussion (0). Sign in to comment.

Pith tools