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Title:Long-term calibration and stability of the Auger Engineering Radio Array using the diffuse Galactic radio emission
Authors:ID de Almeida, R. M. (Author)
ID Filipčič, Andrej (Author)
ID Paul Lundquist, Jonathan (Author)
ID Ujjani Shivashankara, Shima (Author)
ID Stanič, Samo (Author)
ID Vorobiov, Serguei (Author)
ID Zavrtanik, Danilo (Author)
ID Zavrtanik, Marko (Author), et al.
Files:.pdf ICRC2023_279.pdf (1,03 MB)
MD5: AF3B579010AF2948EAB72AC7B77D7EF4
 
URL https://pos.sissa.it/444/
 
URL https://pos.sissa.it/444/279/pdf
 
Language:English
Work type:Not categorized
Typology:1.08 - Published Scientific Conference Contribution
Organization:UNG - University of Nova Gorica
Abstract:The Auger Engineering Radio Array (AERA), part of the Pierre Auger Observatory, is currently the largest facility to measure radio emissions from ultra-high energy extensive air showers. It comprises 153 autonomous radio-detector stations, covering an area of 17 km^2, and measures radio waves in the frequency range from 30 to 80 MHz. An accurate description of the detector response is necessary to interpret the data collected by the stations correctly. Previously, this was achieved by measuring the analog chain in the laboratory and simulating and measuring the directional response of the antenna. In this work, we perform an absolute calibration using the continuously monitored sidereal modulation of the diffuse Galactic radio emission. The calibration is performed by comparing the average spectra recorded by the stations with a model of the full radio sky propagated through the system response, including the antenna, filters, and amplifiers. We describe the method to determine the calibration constants for each antenna and present the corresponding results. Furthermore, the behavior of the calibration constants is studied as a function of time. There is no relevant aging effect over a timescale of a decade, which shows that radio detectors could help monitor possible aging effects of other detector systems during long-term operations, stressing their importance in determining an absolute energy scale.
Keywords:pierre auger observatory, auger engineering radio array, ultra-high energy cosmic rays, radio detectors
Publication status:Published
Publication version:Version of Record
Year of publishing:2023
PID:20.500.12556/RUNG-8787 New window
COBISS.SI-ID:182031875 New window
NUK URN:URN:SI:UNG:REP:WRAUMCZV
Publication date in RUNG:22.01.2024
Views:1782
Downloads:35
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Record is a part of a monograph

Title:38th International Cosmic Ray Conference : ICRC 2023
Place of publishing:Trieste, SISSA
Year of publishing:2023

Document is financed by a project

Funder:ARRS - Slovenian Research Agency
Project number:P1-0031
Name:Večglasniška astrofizika

Licences

License:CC BY-NC-ND 4.0, Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
Link:http://creativecommons.org/licenses/by-nc-nd/4.0/
Description:The most restrictive Creative Commons license. This only allows people to download and share the work for no commercial gain and for no other purposes.

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