© 2014 Elsevier B.V. We describe an experiment using the Parkes radio telescope in the 1.2-1.5 GHz frequency range as part of the LUNASKA project, to search for nanosecond-scale pulses from particle cascades in the Moon, which may be triggered by ultra-high-energy astroparticles. Through the combination of a highly sensitive multi-beam radio receiver, a purpose-built backend and sophisticated signal-processing techniques, we achieve sensitivity to radio pulses with a threshold electric field strength of 0.0053 µV/m/MHz, lower than previous experiments by a factor of three. We observe no pulses in excess of this threshold in observations with an effective duration of 127 h. The techniques we employ, including compensating for the phase, disp...
The lunar Askaryan technique, which involves searching for Askaryan radio pulses from particle casca...
\u3cp\u3eRadio detection of Ultra High Energetic Cosmic Rays and Neutrinos (UHECRv) which hit the Mo...
The lunar technique is a method for maximising the collection area for ultra-high-energy (UHE) cosmi...
Ultra-high-energy cosmic rays, and their expected counterpart neutrinos, are the most energetic part...
© 2015 American Physical Society. We report a limit on the ultrahigh-energy neutrino flux based on a...
The proposal to use ground based radio telescopes for detection of Askaryan radio pulses from partic...
Abstract. This contribution describes the ex-perimental set-up implemented by the LUNASKA project at...
The lunar radio Cherenkov technique uses the moon as a large-volume detector for ultra-high energy (...
The lunar Askaryan technique, which involves searching for Askaryan radio pulses from particle casca...
The use of the Moon as a detector volume for ultra-high-energy neutrinos and cosmic rays, by searchi...
Abstract: A promising method for the detection of UHE neutrinos is the Lunar Cherenkov technique, wh...
The origin of the highest-energy particles in nature, the ultra-high-energy (UHE) cosmic rays, is st...
Low-frequency radio astronomy is limited by severe ionospheric distortions below 50 MHz and complete...
Abstract: Detection of Ultra High Energetic Cosmic Rays and Neutrinos (UHECRv) using the Moon surfac...
The origin of the most energetic particles in nature, the ultra-high-energy (UHE) cosmic rays, is st...
The lunar Askaryan technique, which involves searching for Askaryan radio pulses from particle casca...
\u3cp\u3eRadio detection of Ultra High Energetic Cosmic Rays and Neutrinos (UHECRv) which hit the Mo...
The lunar technique is a method for maximising the collection area for ultra-high-energy (UHE) cosmi...
Ultra-high-energy cosmic rays, and their expected counterpart neutrinos, are the most energetic part...
© 2015 American Physical Society. We report a limit on the ultrahigh-energy neutrino flux based on a...
The proposal to use ground based radio telescopes for detection of Askaryan radio pulses from partic...
Abstract. This contribution describes the ex-perimental set-up implemented by the LUNASKA project at...
The lunar radio Cherenkov technique uses the moon as a large-volume detector for ultra-high energy (...
The lunar Askaryan technique, which involves searching for Askaryan radio pulses from particle casca...
The use of the Moon as a detector volume for ultra-high-energy neutrinos and cosmic rays, by searchi...
Abstract: A promising method for the detection of UHE neutrinos is the Lunar Cherenkov technique, wh...
The origin of the highest-energy particles in nature, the ultra-high-energy (UHE) cosmic rays, is st...
Low-frequency radio astronomy is limited by severe ionospheric distortions below 50 MHz and complete...
Abstract: Detection of Ultra High Energetic Cosmic Rays and Neutrinos (UHECRv) using the Moon surfac...
The origin of the most energetic particles in nature, the ultra-high-energy (UHE) cosmic rays, is st...
The lunar Askaryan technique, which involves searching for Askaryan radio pulses from particle casca...
\u3cp\u3eRadio detection of Ultra High Energetic Cosmic Rays and Neutrinos (UHECRv) which hit the Mo...
The lunar technique is a method for maximising the collection area for ultra-high-energy (UHE) cosmi...