Cosmic ray mass composition measurement in the energy range from $10^{16.5}$ eV to $10^{18.5}$ eV observed with the TALE hybrid detector
Telescope Array Collaboration: R.U. Abbasi (1), T. Abu-Zayyad (1,2), M. Allen (2), J.W. Belz (2), D.R. Bergman (2), F. Bradfield (3), I. Buckland (2), W. Campbell (2), B.G. Cheon (4), K. Endo (3), A. Fedynitch (5,6), T. Fujii (3,7), K. Fujisue (5,6), K. Fujita (5)

TL;DR
This study measures cosmic ray composition using the TALE hybrid detector, revealing a transition from heavy to lighter nuclei around 10^17 eV, indicating a shift from Galactic to extragalactic sources.
Contribution
First detailed measurement of cosmic ray mass composition in the 10^16.5 to 10^18.5 eV range with the TALE hybrid detector, showing a composition transition around 10^17 eV.
Findings
Elongation rate exhibits a break near 10^17 eV.
Composition becomes heavier up to 10^17 eV, then lighter beyond.
Results support a Galactic to extragalactic transition around the second knee.
Abstract
We report on the cosmic ray mass composition measured by the Telescope Array Low-energy Extension (TALE) hybrid detector. The TALE detector consists of a fluorescence detector (FD) station with 10 FD telescopes located at the Telescope Array (TA) Middle Drum FD Station (itself made up of 14 FD telescopes), and a surface detector (SD) array of scintillators. The array consists of 40 SDs with 400 m spacing and 40 SDs with 600 m spacing. In this paper, we present results on the measurement of the depth of shower maxima () in the energy range from eV to eV collected over five years of the TALE hybrid detector. The distributions were analyzed and compared with Monte Carlo simulations of proton, helium, nitrogen, and iron primaries, using the QGSJet II-04 hadronic interaction model. Our results indicate that the elongation rate of the…
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