Authors

O. Adriani, Università degli Studi di Firenze
Y. Akaike, Waseda University
K. Asano, The University of Tokyo
Y. Asaoka, The University of Tokyo
E. Berti, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
P. Betti, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
G. Bigongiari, Università degli Studi di Siena
W. R. Binns, McDonnell Center for the Space Sciences
M. Bongi, Università degli Studi di Firenze
P. Brogi, Università degli Studi di Siena
A. Bruno, NASA Goddard Space Flight Center
N. Cannady, NASA Goddard Space Flight Center
G. Castellini, Istituto Di Fisica Applicata Nello Carrara
C. Checchia, Università degli Studi di Siena
M. L. Cherry, Louisiana State University
G. Collazuol, Università degli Studi di Padova
G. A. de Nolfo, NASA Goddard Space Flight Center
K. Ebisawa, JAXA Institute of Space and Astronautical Science
A. W. Ficklin, Louisiana State University
H. Fuke, JAXA Institute of Space and Astronautical Science
S. Gonzi, Università degli Studi di Firenze
T. G. Guzik, Louisiana State University
T. Hams, College of Engineering and Information Technology
K. Hibino, Kanagawa University
M. Ichimura, Hirosaki University
M. H. Israel, McDonnell Center for the Space Sciences
K. Kasahara, Shibaura Institute of Technology
J. Kataoka, Waseda University
R. Kataoka, National Institute of Polar Research
Y. Katayose, Yokohama National University
C. Kato, Shinshu University
N. Kawanaka, Tokyo Metropolitan University
Y. Kawakubo, Aoyama Gakuin University

Document Type

Article

Publication Date

7-11-2025

Abstract

The Calorimetric Electron Telescope (CALET), in operation on the International Space Station since 2015, collected a large sample of cosmic-ray (CR) iron and sub-iron events over a wide energy interval. In this Letter, we report an update of our previous measurement of the iron flux and we present-for the first time-a high statistics measurement of the spectra of two sub-iron elements Cr and Ti in the energy interval from 10 to 250  GeV/n. The analyses are based on 8 years of data. Differently from older generations of cosmic-ray instruments which, in most cases, could not resolve individual sub-iron elements, CALET can identify each nuclear species from proton to nickel (and beyond) with a measurement of their electric charge. Thanks to the improvement in statistics and a more refined assessment of systematic uncertainties, the iron spectral shape is better resolved, at high energy, than in our previous paper, and we report its flux ratio to chromium and titanium. The measured fluxes of Cr and Ti show energy dependences compatible with a single power law with spectral indices -2.74±0.06 and -2.88±0.06, respectively.

Publication Source (Journal or Book title)

Physical Review Letters

First Page

021002

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