Search for short bursts of gamma rays with SGARFACE

M. Schroedter; H. Manseri; S. Lebohec; F. Krennrich; C. Dowdall; A. Falcone; S. Fegan; D. Horan; A. Smith; J. Toner; T. Weekes

Search for short bursts of gamma rays with SGARFACE

M. Schroedter
, H. Manseri
, S. Lebohec
, F. Krennrich
, C. Dowdall
, A. Falcone
, S. Fegan
, D. Horan
, A. Smith
, J. Toner
, T. Weekes

Iowa State University
University of Utah
University College Dublin
Pennsylvania State University
University of California, Los Angeles
Argonne National Laboratory
University of Leeds
Center for Astrophysics | Harvard & Smithsonian

Résultats de recherche: Contribution à une conférence › Papier › Revue par des pairs

Résumé

The Short GAmma Ray Front Air Cherenkov Experiment (SGARFACE) is designed to search for bursts of γ rays above 200 MeV lasting from 1 ns to 16 μs. The custom-designed trigger and dataacquisition system is coupled to the camera on the Whipple 10m telescope, an air-Cherenkov telescope in southern Arizona. The experiment has operated for more than 3 years during which time about 1 million events were recorded. Rejection of the cosmic-ray background and of atmospheric phenomena is accomplished through time-resolved imaging of the recorded Cherenkov light. Potential sources of bursts of γ rays are the final explosion of primordial black holes within about 200 pc and γ-ray emission accompanying giant radio pulses. Results of the search for explosions of primordial black holes will be given in a future publication.

langue originale	Anglais
Pages	783-786
Nombre de pages	4
état	Publié - 1 janv. 2007
Modification externe	Oui
Evénement	30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexique Durée: 3 juil. 2007 → 11 juil. 2007

Une conférence

Une conférence	30th International Cosmic Ray Conference, ICRC 2007
Pays/Territoire	Mexique
La ville	Merida, Yucatan
période	3/07/07 → 11/07/07

Contient cette citation

@conference{70c5948f2def480397fc74a3eee383dd,

title = "Search for short bursts of gamma rays with SGARFACE",

abstract = "The Short GAmma Ray Front Air Cherenkov Experiment (SGARFACE) is designed to search for bursts of γ rays above 200 MeV lasting from 1 ns to 16 μs. The custom-designed trigger and dataacquisition system is coupled to the camera on the Whipple 10m telescope, an air-Cherenkov telescope in southern Arizona. The experiment has operated for more than 3 years during which time about 1 million events were recorded. Rejection of the cosmic-ray background and of atmospheric phenomena is accomplished through time-resolved imaging of the recorded Cherenkov light. Potential sources of bursts of γ rays are the final explosion of primordial black holes within about 200 pc and γ-ray emission accompanying giant radio pulses. Results of the search for explosions of primordial black holes will be given in a future publication.",

author = "M. Schroedter and H. Manseri and S. Lebohec and F. Krennrich and C. Dowdall and A. Falcone and S. Fegan and D. Horan and A. Smith and J. Toner and T. Weekes",

year = "2007",

month = jan,

day = "1",

language = "English",

pages = "783--786",

note = "30th International Cosmic Ray Conference, ICRC 2007 ; Conference date: 03-07-2007 Through 11-07-2007",

}

TY - CONF

T1 - Search for short bursts of gamma rays with SGARFACE

AU - Schroedter, M.

AU - Manseri, H.

AU - Lebohec, S.

AU - Krennrich, F.

AU - Dowdall, C.

AU - Falcone, A.

AU - Fegan, S.

AU - Horan, D.

AU - Smith, A.

AU - Toner, J.

AU - Weekes, T.

PY - 2007/1/1

Y1 - 2007/1/1

N2 - The Short GAmma Ray Front Air Cherenkov Experiment (SGARFACE) is designed to search for bursts of γ rays above 200 MeV lasting from 1 ns to 16 μs. The custom-designed trigger and dataacquisition system is coupled to the camera on the Whipple 10m telescope, an air-Cherenkov telescope in southern Arizona. The experiment has operated for more than 3 years during which time about 1 million events were recorded. Rejection of the cosmic-ray background and of atmospheric phenomena is accomplished through time-resolved imaging of the recorded Cherenkov light. Potential sources of bursts of γ rays are the final explosion of primordial black holes within about 200 pc and γ-ray emission accompanying giant radio pulses. Results of the search for explosions of primordial black holes will be given in a future publication.

AB - The Short GAmma Ray Front Air Cherenkov Experiment (SGARFACE) is designed to search for bursts of γ rays above 200 MeV lasting from 1 ns to 16 μs. The custom-designed trigger and dataacquisition system is coupled to the camera on the Whipple 10m telescope, an air-Cherenkov telescope in southern Arizona. The experiment has operated for more than 3 years during which time about 1 million events were recorded. Rejection of the cosmic-ray background and of atmospheric phenomena is accomplished through time-resolved imaging of the recorded Cherenkov light. Potential sources of bursts of γ rays are the final explosion of primordial black holes within about 200 pc and γ-ray emission accompanying giant radio pulses. Results of the search for explosions of primordial black holes will be given in a future publication.

M3 - Paper

AN - SCOPUS:84899507074

SP - 783

EP - 786

T2 - 30th International Cosmic Ray Conference, ICRC 2007

Y2 - 3 July 2007 through 11 July 2007

ER -

Search for short bursts of gamma rays with SGARFACE

Résumé

Une conférence

Empreinte digitale

Contient cette citation