Detecting and monitoring emissions from flaring gamma-ray sources in the very-high-energy (VHE, >100 GeV) band is a very important topic in gamma-ray astronomy. The ARGO-YBJ detector is characterized by a high duty cycle and a wide field of view. Therefore, it is particularly capable of detecting flares from extragalactic objects. Based on fast reconstruction and analysis, real-time monitoring of 33 selected VHE extragalactic sources is implemented. Flares exceeding a specific threshold are reported timely, hence enabling the follow-up observation of these objects using more sensitive detectors, such as Cherenkov telescopes.

Bartoli, B., Bernardini, P., Bi, X.J., Bleve, C., Bolognino, I., Branchini, P., et al. (2011). Early warning for VHE gamma-ray flares with the ARGO-YBJ detector. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH. SECTION A, ACCELERATORS, SPECTROMETERS, DETECTORS AND ASSOCIATED EQUIPMENT, 659(1), 428-433 [doi:10.1016/j.nima.2011.09.013].

Early warning for VHE gamma-ray flares with the ARGO-YBJ detector

D'ALI'STAITI, Giacomo;Marsella, G;
2011-01-01

Abstract

Detecting and monitoring emissions from flaring gamma-ray sources in the very-high-energy (VHE, >100 GeV) band is a very important topic in gamma-ray astronomy. The ARGO-YBJ detector is characterized by a high duty cycle and a wide field of view. Therefore, it is particularly capable of detecting flares from extragalactic objects. Based on fast reconstruction and analysis, real-time monitoring of 33 selected VHE extragalactic sources is implemented. Flares exceeding a specific threshold are reported timely, hence enabling the follow-up observation of these objects using more sensitive detectors, such as Cherenkov telescopes.
2011
Bartoli, B., Bernardini, P., Bi, X.J., Bleve, C., Bolognino, I., Branchini, P., et al. (2011). Early warning for VHE gamma-ray flares with the ARGO-YBJ detector. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH. SECTION A, ACCELERATORS, SPECTROMETERS, DETECTORS AND ASSOCIATED EQUIPMENT, 659(1), 428-433 [doi:10.1016/j.nima.2011.09.013].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/63234
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