| Title: | Status and expected performance of the AugerPrime radio detector |
|---|
| Authors: | ID Pawlowsky, Jannis (Author)
ID Filipčič, Andrej (Author)
ID Lundquist, Jon Paul (Author)
ID Shivashankara, Shima Ujjani (Author)
ID Stanič, Samo (Author)
ID Vorobiov, Serguei (Author)
ID Zavrtanik, Danilo (Author)
ID Zavrtanik, Marko (Author), et al. |
|---|
| Files: |  ICRC2023_344.pdf (7,29 MB)
MD5: FCDC0184B77DD8C63445F731485B77EA
 https://pos.sissa.it/444/
https://pos.sissa.it/444/344/pdf
|
|---|
| Language: | English |
|---|
| Work type: | Unknown |
|---|
| Typology: | 1.08 - Published Scientific Conference Contribution |
|---|
| Organization: | UNG - University of Nova Gorica
|
|---|
| Abstract: | The ongoing AugerPrime upgrade of the Pierre Auger Observatory will yield sensitivity and precision for measuring ultra-high energy (UHE) cosmic rays that are significantly improved over the baseline design. A key part is the installation of the Radio Detector (RD), consisting
of loop antennas mounted on top of each of the 1660 water-Cherenkov detectors (WCD). These antennas, with polarizations both parallel and perpendicular to Earth’s magnetic field, are sensitive to inclined air showers and will also improve the sky coverage and exposure of the observatory. Of special interest is the great sensitivity to the electromagnetic component of air showers, yielding new information for the reconstruction of the primary mass, energy and arrival direction. Complementing traditional particle detectors like the WCD, the combination of both yields new opportunities to detect rare primary particles, e.g. UHE photons and neutrinos with a large
identification probability.
Here we present the status and future prospects of the RD.With mass production and deployment ongoing, we showair shower statistics and reconstructions of the already installed detector stations.
We detail the layout and integration of the RD, demonstrating the potential of the observatory including radio measurements and RD triggering, especially to detect air showers with weak particle footprints. We show that the new trigger enables the measurement of events for which traditional particle detectors are less sensitive. |
|---|
| Keywords: | ultra-high energy cosmic rays, Pierre Auger Observatory, radio detector, air shower |
|---|
| Publication status: | Published |
|---|
| Publication version: | Version of Record |
|---|
| Publication date: | 01.01.2023 |
|---|
| Year of publishing: | 2023 |
|---|
| Number of pages: | str. 1-13 |
|---|
| PID: | 20.500.12556/RUNG-8795  |
|---|
| COBISS.SI-ID: | 182094851 |
|---|
| UDC: | 52 |
|---|
| ISSN on article: | 1824-8039 |
|---|
| DOI: | 10.22323/1.444.0344 |
|---|
| NUK URN: | URN:SI:UNG:REP:5NRRA0CM |
|---|
| Publication date in RUNG: | 23.01.2024 |
|---|
| Views: | 1250 |
|---|
| Downloads: | 6 |
|---|
| Metadata: |    |
|---|
|
:
|
Copy citation |
|---|
| | | | Average score: | (0 votes) |
|---|
| Your score: | Voting is allowed only for logged in users. |
|---|
| Share: |  |
|---|
Hover the mouse pointer over a document title to show the abstract or click
on the title to get all document metadata. |
