Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/40239
Title: Investigating the nature of the INTEGRAL gamma-ray bursts and sub-threshold triggers with Swift follow-up
Authors: Higgins, A. B.
Starling, Rhaana Leigh Catherine
Götz, D.
Mereghetti, S.
Wiersema, K.
Maccarone, T.
Osborne, J. P.
Tanvir, N. R.
O'Brien, P. T.
Bird, A. J.
Rowlinson, A.
Gehrels, N.
First Published: 12-May-2017
Publisher: Oxford University Press on behalf of the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2017, 470 (1), pp. 314-323
Abstract: 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, IGRW151019, 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.
DOI Link: 10.1093/mnras/stx1163
ISSN: 0035-8711
eISSN: 1365-2966
Links: https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stx1163
http://hdl.handle.net/2381/40239
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2017, the author(s). Deposited with reference to the publisher’s open access archiving policy.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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