Short gamma-ray bursts within 200 Mpc
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Date
2020-01-21
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Dichiara, S.; Troja, E.; O’Connor, B.; Marshall, F. E.; Beniamini, P.; Cannizzo, J. K.; Lien, A. Y.; Sakamoto, T.; Short gamma-ray bursts within 200 Mpc; High Energy Astrophysical Phenomena (2019); https://arxiv.org/abs/1912.08698
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Abstract
We present a systematic search for short-duration gamma-ray bursts (GRBs) in the local Universe based on 14 years of observations with the Neil Gehrels Swift Observatory. We cross-correlate the GRB positions with the GLADE catalogue of nearby galaxies, and find no event at a distance ≲100 Mpc and four plausible candidates in the range 100 Mpc≲D≲200 Mpc. Although affected by low statistics, this number is higher than the one expected for chance alignments to random galaxies, and possibly suggests a physical association between these bursts and nearby galaxies. By assuming a local origin, we use these events to constrain the range of properties for X-ray counterparts of neutron star mergers. Optical upper limits place tight constraints on the onset of a blue kilonova, and imply either low masses (≲10⁻³M⊙) of lanthanide-poor ejecta or unfavorable orientations (θobs≳30 deg). Finally, we derive that the all-sky rate of detectable short GRBs within 200 Mpc is 1.3+1.7−0.8 yr⁻¹ (68\% confidence interval), and discuss the implications for the GRB outflow structure. If these candidates are instead of cosmological origin, we set a upper limit of ≲2.0 yr⁻¹ (90\% confidence interval) to the rate of nearby events detectable with operating gamma-ray observatories, such as Swift and Fermi.