Prospects for VHE monitoring of gamma-ray bursts with SWGO

被引:0
作者
La Mura, G. [1 ]
Barres de Almeida, U. [2 ]
Conceicao, R. [1 ,3 ]
de Angelis, A. [4 ,5 ,6 ]
Longo, F. [7 ,8 ,9 ]
Pimenta, M. [1 ,3 ]
Prandini, E. [6 ,10 ]
Ruiz-Velasco, E. [11 ]
Tome, B. [1 ,3 ]
机构
[1] Lab Instrumentacao & Fis Expt Particulas LIP, Ave Prof Gama Pinto 2, P-1649003 Lisbon, Portugal
[2] Brazilian Ctr Phys Res CBPF, Rua Dr Xavier Sigaud 150, BR-22290180 Rio De Janeiro, Brazil
[3] IST, Ave Rovisco Pais 1, P-1049001 Lisbon, Portugal
[4] Univ Padua, Dipartimento Fis & Astron, Via Marzolo 8, I-35131 Padua, Italy
[5] Univ Udine, Dipartimento Sci Matemat Informat & Fis, Via Palladio 8, I-33100 Udine, Italy
[6] Ist Nazl Fis Nucl Sez Padova INFN, Via Marzolo 8, I-35131 Padua, Italy
[7] IFPU, Via Beirut 2, I-34014 Trieste, Italy
[8] Ist Nazl Fis Nucl, Sez Trieste, Via A Valerio 2, I-34100 Trieste, Italy
[9] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34100 Trieste, Italy
[10] INAF Osservatorio Astron Padova, Vicolo Osservatorio 3, I-35122 Padua, Italy
[11] Max Planck Inst Kernphys, POB 103980, D-69029 Heidelberg, Germany
来源
SIXTEENTH MARCEL GROSSMANN MEETING | 2023年
关键词
Instrumentation: detectors; gamma rays: general; gamma ray burst: general; FERMI OBSERVATIONS; COMPONENT; MODELS; SUPERNOVA; PHOTONS; SPECTRA;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It has been established that Gamma-Ray Bursts (GRB) can produce Very High Energy radiation (VHE, E > 100 GeV), opening a new window for investigating particle acceleration and radiation properties in the most energetic domain. We expect that next-generation instruments in this energy regime, such as the Cherenkov Telescope Array (CTA), will mark a huge improvement in their observation. However, constraints on the target visibility and the limited duty cycle of Imaging Atmospheric Cherenkov Telescopes (IACT), affect their ability to react promptly to transient events. Here we use a grid of instrument performance estimates, based on the Extensive Air Shower (EAS) array concept proposed by the Southern Wide Field-of-view Gamma-ray Observatory (SWGO) collaboration, to evaluate SWGO's potential to detect and track VHE emission from GRBs. Observations by the Fermi Large Area Telescope (Fermi-LAT) at high energy (E > 10 GeV), identified some events with a distinct spectral component, which can represent a substantial fraction of the emitted energy and possibly occur very early in the process. Using models based on these properties, we estimate the possibilities that a wide field of view and large effective area ground-based monitoring facility has to probe VHE emission from GRBs. We show that the ability to monitor VHE transients with a nearly continuous scanning of the sky grants us the opportunity to simultaneously observe electromagnetic counterparts to gravitational waves and relativistic particles sources up to cosmological scales, in a way that is not accessible to IACTs.
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页码:3041 / 3051
页数:11
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