Energy calibration of LHAASO-KM2A using the cosmic ray Moon shadow

preprint2026arXivOpen access
Zhen CaoF. AharonianY. X. BaiY. W. BaoD. BastieriX. J. BiY. J. BiW. BianJ. BlunierA. V. BukevichC. M. CaiY. Y. CaiW. Y. CaoZhe CaoJ. ChangJ. F. ChangE. S. ChenG. H. ChenH. K. ChenL. F. ChenLiang ChenLong ChenM. J. ChenM. L. ChenQ. H. ChenS. ChenS. H. ChenS. Z. ChenT. L. ChenX. B. ChenX. J. ChenX. P. ChenY. ChenN. ChengQ. Y. ChengY. D. ChengM. Y. CuiS. W. CuiX. H. CuiY. D. CuiB. Z. DaiH. L. DaiZ. G. DaiDanzengluobuY. X. DiaoA. J. DongX. Q. DongK. K. DuanJ. H. FanY. Z. FanJ. FangJ. H. FangK. FangC. F. FengH. FengL. FengS. H. FengX. T. FengY. FengY. L. FengS. GabiciB. GaoQ. GaoW. GaoW. K. GaoM. M. GeT. T. GeL. S. GengG. GiacintiG. H. GongQ. B. GouM. H. GuF. L. GuoJ. GuoK. J. GuoX. L. GuoY. Q. GuoY. Y. GuoR. P. HanO. A. HannukselaM. HasanH. H. HeH. N. HeJ. Y. HeX. Y. HeY. HeS. Hernández-CadenaB. W. HouC. HouX. HouH. B. HuS. C. HuC. HuangD. H. HuangJ. J. HuangX. L. HuangX. T. HuangX. Y. HuangY. HuangY. Y. HuangA. InventarX. L. JiH. Y. JiaK. JiaH. B. JiangK. JiangX. W. JiangZ. J. JiangM. JinS. KaciM. M. KangI. KarpikovD. KhangulyanD. KuleshovK. KurinovCheng LiCong LiD. LiF. LiH. B. LiH. C. LiJian LiJie LiK. LiL. LiR. L. LiS. D. LiT. Y. LiW. L. LiX. R. LiXin LiY. LiZhe LiZhuo LiE. W. LiangY. F. LiangS. J. LinB. LiuC. LiuD. LiuD. B. LiuH. LiuJ. LiuJ. L. LiuJ. R. LiuM. Y. LiuR. Y. LiuS. M. LiuW. LiuX. LiuY. LiuY. N. LiuY. Q. LouQ. LuoY. LuoH. K. LvB. Q. MaL. L. MaX. H. MaI. O. MaliyJ. R. MaoZ. MinW. MitthumsiriY. MizunoG. B. MouA. NeronovK. C. Y. NgM. Y. NiL. NieL. J. OuZ. W. OuP. PattarakijwanichZ. Y. PeiD. Y. PengJ. C. QiM. Y. QiJ. J. QinD. QuA. RazaC. Y. RenD. RuffoloA. SáizD. SavchenkoD. SemikozL. ShaoO. ShchegolevY. Z. ShenX. D. ShengZ. D. ShiF. W. ShuH. C. SongYu. V. StenkinV. StepanovY. SuD. X. SunH. SunJ. X. SunQ. N. SunX. N. SunZ. B. SunN. H. TabasamJ. TakataP. H. T. TamH. B. TanQ. W. TangR. TangZ. B. TangW. W. TianC. N. TongL. H. WanC. WangD. H. WangG. W. WangH. G. WangJ. C. WangK. WangKai WangL. P. WangL. Y. WangR. WangW. WangX. G. WangX. J. WangX. Y. WangY. WangY. D. WangZ. H. WangZ. X. WangZheng WangD. M. WeiJ. J. WeiY. J. WeiT. WenS. S. WengC. Y. WuH. R. WuQ. W. WuS. WuX. F. WuY. S. WuS. Q. XiJ. XiaJ. J. XiaG. M. XiangD. X. XiaoG. XiaoY. F. XiaoY. L. XinH. D. XingY. XingD. R. XiongB. N. XuC. Y. XuD. L. XuR. F. XuR. X. XuS. S. XuW. L. XuL. XueD. H. YanT. YanC. W. YangC. Y. YangF. F. YangL. L. YangM. J. YangR. Z. YangW. X. YangZ. H. YangZ. G. YaoX. A. YeL. Q. YinN. YinX. H. YouZ. Y. YouQ. YuanH. YueH. D. ZengT. X. ZengW. ZengX. T. ZengM. ZhaB. B. ZhangB. T. ZhangC. ZhangH. ZhangH. M. ZhangH. Y. ZhangJ. L. ZhangJ. Y. ZhangLi ZhangP. F. ZhangR. ZhangS. R. ZhangS. S. ZhangS. Y. ZhangW. ZhangW. Y. ZhangX. ZhangX. P. ZhangYi ZhangYong ZhangZ. P. ZhangJ. ZhaoL. ZhaoL. Z. ZhaoS. P. ZhaoX. H. ZhaoZ. H. ZhaoF. ZhengT. C. ZhengB. ZhouH. ZhouJ. N. ZhouM. ZhouP. ZhouR. ZhouX. X. ZhouB. Y. ZhuC. G. ZhuF. R. ZhuH. ZhuK. J. ZhuY. C. ZouX. ZuoFaisal Akram

Abstract

We present a precise measurement of the westward, rigidity-dependent shift of the Moon's shadow using three and a half years of cosmic-ray data collected by the Kilometer Square Array (KM2A) of the Large High Altitude Air Shower Observatory (LHAASO). These measurements enable us to calibrate the detector energy response in the range 20-260 TeV, with results showing excellent agreement with the response derived from Monte Carlo (MC) simulations of the KM2A detector. We also measure a best-fit parameter ε=0.015±0.08ε= 0.015 \pm 0.08, corresponding to a 95% confidence interval of [-14%, +17%] for the energy-scale estimation. This result establishes the exceptional accuracy of the KM2A-MC in simulating the detector's response within this energy range.

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