Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory
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- Nijmegen U., IMAPP
- LIP, Lisbon
- Turin Observ.; INFN, Turin
- Sao Paulo U.
- Adelaide U.
- Centro Atomico Bariloche
- ITeDA, Buenos Aires; U. Tech. Natl., Argentina
- Mexico U.
- Santiago de Compostela U.
- INFN, Aquila; Gran Sasso
- Lehman Coll.
- ITeDA, Buenos Aires
- INFN, Naples
- Bucharest, Inst. Space Science
- Centro Atomico Bariloche; Cantabria U., Santander
- Pierre Auger Observ.
- Bucharest, Polytechnic Inst.
- Bucharest, IFIN-HH
- Naples U.; INFN, Naples
- KIT, Karlsruhe, IKP
- Wuppertal U.
- LPSC, Grenoble
- Turin U.; INFN, Turin
- Orsay, IPN
- Prague, Inst. Phys.
- Salento U.; INFN, Lecce
- Rio de Janeiro Federal U.
- Cracow, INP
- ITeDA, Buenos Aires; KIT, Karlsruhe, IKP
- Aachen, Tech. Hochsch.
- KIT, Karlsruhe, ETP
- Siegen U.
- Granada U., Theor. Phys. Astrophys.
- Catania U.; INFN, Catania
- Chiapas Autonoma U.
- Milan U.
- La Plata U.
- U. Tech. Natl., Argentina; ITeDA, Buenos Aires
- Nijmegen U., IMAPP; Nikhef, Amsterdam
- U. Sao Paulo (main)
- INFN, Lecce
- Campinas State U.
- Palacky U.
- Natl. Tech. U., San Rafael
- Penn State U.
- INFN, Turin
- INFN, Milan; Milan Polytechnic
- Case Western Reserve U.
- Salento U., DII; INFN, Lecce
- Buenos Aires, IAFE; Buenos Aires U.
- Niteroi, Fluminense U.
- Sao Paulo U., Sao Carlos
- Parana U.
- Hamburg U., Inst. Theor. Phys. II
- Fermilab
- Nijmegen U., IMAPP; ASTRON, Dwingeloo; Nikhef, Amsterdam
- Chicago U., EFI
- New York U.
- KIT, Karlsruhe, IPE
- Michigan Tech. U.
- Stefan Inst., Ljubljana; Nova Gorica U.
- IFIR, Rosario
- Paris U., VI-VII
- Rio de Janeiro Federal U.; Rio de Janeiro, CBPF
- INFN, Milan
- U. Lodz (main)
- Centro Atomico Bariloche; KIT, Karlsruhe, IKP
- UEFS, Feira de Santana
- INFN, Turin; Turin U.
- KIT, Karlsruhe, ETP; ITeDA, Buenos Aires
- Colorado School of Mines
- Nova Gorica U.
- ABC Federal U.
- Puebla U., Inst. Fis.
- Milan U.; INFN, Milan
- Brussels U.
- CINVESTAV, IPN
- Louisiana State U.
- Rome U., Tor Vergata; INFN, Rome2
- Charles U.
- Cantabria U., Santander
- LIDAR CITEFA
- UPII, IPN
- L'Aquila U.; Gran Sasso
- Buenos Aires, IAFE
- INFN, Rome2
- KIT, Karlsruhe, IKP; ITeDA, Buenos Aires
- Groningen, KVI
- Palermo Observ.; INFN, Catania
- Rio de Janeiro, CBPF
- Nebraska U.
- Northeastern U.
- Nikhef, Amsterdam; Nijmegen U., IMAPP
- Nova Gorica U.; Stefan Inst., Ljubljana
With the Auger Engineering Radio Array (AERA) of the Pierre Auger Observatory, we have observed the radio emission from 561 extensive air showers with zenith angles between 60o and 84o. In contrast to air showers with more vertical incidence, these inclined air showers illuminate large ground areas of several km2 with radio signals detectable in the 30 to 80 MHz band. A comparison of the measured radio-signal amplitudes with Monte Carlo simulations of a subset of 50 events for which we reconstruct the energy using the Auger surface detector shows agreement within the uncertainties of the current analysis. As expected for forward-beamed radio emission undergoing no significant absorption or scattering in the atmosphere, the area illuminated by radio signals grows with the zenith angle of the air shower. Inclined air showers with EeV energies are thus measurable with sparse radio-antenna arrays with grid sizes of a km or more. This is particularly attractive as radio detection provides direct access to the energy in the electromagnetic cascade of an air shower, which in case of inclined air showers is not accessible by arrays of particle detectors on the ground.
- Research Organization:
- ABC Federal U.; ASTRON, Dwingeloo; Aachen, Tech. Hochsch.; Adelaide U.; Brussels U.; Bucharest, IFIN-HH; Bucharest, Inst. Space Science; Bucharest, Polytechnic Inst.; Buenos Aires U.; Buenos Aires, IAFE; CINVESTAV, IPN; Campinas State U.; Cantabria U., Santander; Case Western Reserve U.; Catania U.; Centro Atomico Bariloche; Charles U.; Chiapas Autonoma U.; Chicago U., EFI; Colorado School of Mines; Cracow, INP; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Gran Sasso; Granada U., Theor. Phys. Astrophys.; Groningen, KVI; Hamburg U., Inst. Theor. Phys. II; IFIR, Rosario; INFN, Aquila; INFN, Catania; INFN, Lecce; INFN, Milan; INFN, Naples; INFN, Rome2; INFN, Turin; ITeDA, Buenos Aires; KIT, Karlsruhe, ETP; KIT, Karlsruhe, IKP; KIT, Karlsruhe, IPE; L'Aquila U.; LIDAR CITEFA; LIP, Lisbon; LPSC, Grenoble; La Plata U.; Lehman Coll.; Louisiana State U.; Mexico U.; Michigan Tech. U.; Milan Polytechnic; Milan U.; Naples U.; Natl. Tech. U., San Rafael; Nebraska U.; New York U.; Nijmegen U., IMAPP; Nikhef, Amsterdam; Niteroi, Fluminense U.; Northeastern U.; Nova Gorica U.; Orsay, IPN; Palacky U.; Palermo Observ.; Parana U.; Paris U., VI-VII; Penn State U.; Pierre Auger Observ.; Prague, Inst. Phys.; Puebla U., Inst. Fis.; Rio de Janeiro Federal U.; Rio de Janeiro, CBPF; Rome U., Tor Vergata; Salento U.; Salento U., DII; Santiago de Compostela U.; Sao Paulo U.; Sao Paulo U., Sao Carlos; Siegen U.; Stefan Inst., Ljubljana; Turin Observ.; Turin U.; U. Lodz (main); U. Sao Paulo (main); U. Tech. Natl., Argentina; UEFS, Feira de Santana; UPII, IPN; Wuppertal U.
- Sponsoring Organization:
- US Department of Energy
- Grant/Contract Number:
- AC02-07CH11359
- OSTI ID:
- 1463631
- Report Number(s):
- FERMILAB-PUB-18-259-ND; oai:inspirehep.net:1677962; arXiv:1806.05386
- Journal Information:
- JCAP, Journal Name: JCAP Vol. 10
- Country of Publication:
- United States
- Language:
- English
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