This data is released under CC BY-SA 4.0. All Auger Open Data have a DOI that you are requested to cite in any applications or publications. The data published here is part of the main dataset, http://doi.org/10.5281/zenodo.4487612. Also consider whether citing the release paper, 2023arXiv230916294T, is appropriate.
The data was obtained from https://zenodo.org/records/10488964, where you will also find additional material.
Delivery service for the full event files. To query the data, use TAP on http://dc.g-vo.org/tap and inspect the auger3 schema.
Highly inclined (60 to 80°) Auger public events detected by the surface detectors in all configurations.
Auger public events detected by the surface detectors in the SD1500 configuration.
Auger public events detected by the surface detectors in the SD750 configuration.
For every Auger station during every second, the scalers record the number of times that the amplitude of the signal is larger than 3 ADC counts, corresponding to an energy deposit of about 15 MeV, and smaller than 21 ADC counts, corresponding to an energy deposit of about 100 MeV.
This table allows one to study the temporal behavior of the number of counts, which is modulated by terrestrial and extraterrestrial phenomena.
This data is released under CC BY-SA 4.0. All Auger Open Data have a DOI that you are requested to cite in any applications or publications. The data published here is part of the main dataset, http://doi.org/10.5281/zenodo.4487612. Also consider whether citing the release paper, 2023arXiv230916294T, is appropriate.
The data was obtained from https://zenodo.org/records/10488964, where you will also find additional material.
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