Measurement of the cosmic ray spectrum with the Pierre Auger Observatory

被引：0

作者：

Mockler, Daniela ^{[1
]}

机构：

[1] Karlsruhe Inst Technol, Inst Expt Particle Phys ETP, Karlsruhe, Germany

来源：

7TH ROMA INTERNATIONAL CONFERENCE ON ASTROPARTICLE PHYSICS (RICAP18) | 2019年 / 209卷

关键词：

DETECTOR; SHOWERS;

D O I：

10.1051/epjconf/201920901029

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The flux of ultra-high energy cosmic rays above 3 x 10(17) eV has been measured with unprecedented precision at the Pierre Auger Observatory. The flux of the cosmic rays is determined by four different measurements. The surface detector array provides three data sets, two formed by dividing the data into two zenith angle ranges, and one obtained from a nested, denser detector array. The fourth measurement is obtained with the fluorescence detector. By combing all four data sets, the all-sky flux of cosmic rays is determined. The spectral features are discussed in detail and systematic uncertainties are addressed.

引用

页数：4

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