Investigating the nature of the INTEGRAL gamma-ray bursts and sub-threshold triggers with Swift follow-up
Investigating the nature of the INTEGRAL gamma-ray bursts and sub-threshold triggers with Swift follow-up
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DOI:
10.1093/mnras/stx1163
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发表时间:
2017-05
影响因子:
4.8
通讯作者:
A. Higgins;R. Starling;D. Gotz;S. Mereghetti;K. Wiersema;T. Maccarone;J. Osborne;N. Tanvir;P. O’Brien;A. Bird;A. Rowlinson;N. Gehrels
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文献类型:
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作者:
A. Higgins;R. Starling;D. Gotz;S. Mereghetti;K. Wiersema;T. Maccarone;J. Osborne;N. Tanvir;P. O’Brien;A. Bird;A. Rowlinson;N. Gehrels
We explore the potential of the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) to improve our understanding of the low-fluence regime for explosive transients, such as Gamma-ray Bursts (GRBs). We probe the nature of the so-called 'WEAK' INTEGRAL triggers, when the gamma-ray instruments record intensity spikes that are below the usual STRONG significance thresholds. In a targeted Swift follow-up campaign, we observed 15 WEAK triggers. We find six of these can be classified as GRBs. This includes GRB 150305A, a GRB discovered from our campaign alone. We also identified a source coincident with one trigger, IGRW 151019, as a candidate active galactic nucleus. We show that real events such as GRBs exist within the INTEGRAL Burst Alert System (IBAS) WEAK trigger population. A comparison of the fluence distributions of the full INTEGRAL IBAS and Swift-BAT GRB samples showed that the two are similar. We also find correlations between the prompt gamma-ray and X-ray properties of the two samples, supporting previous investigations. We find that both satellites reach similar, low fluence levels regularly, although Swift is more sensitive to short, low-fluence GRBs.