An origin for short γ-ray bursts unassociated with current star formation
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P. Giommi | T. Sakamoto | A. Melandri | P. D'Avanzo | P. T. O'Brien | D. N. Burrows | S. Kobayashi | G. Tagliaferri | S. Campana | J. A. Nousek | S. Covino | S. D. Barthelmy | M. B. Davies | J. A. Kennea | L. A. Antonelli | C. Kouveliotou | N. Gehrels | D. Grupe | G. Chincarini | A. Moretti | P. Romano | S. Vaughan | T. Sakamoto | S. Barthelmy | C. Kouveliotou | N. Gehrels | D. Burrows | P. Giommi | P. O’Brien | A. Melandri | D. Grupe | J. Nousek | A. Moretti | G. Tagliaferri | A. King | M. Goad | M. Davies | G. Chincarini | J. Kennea | S. Vaughan | S. Covino | P. D’Avanzo | Bing Zhang | P. Mészáros | P. Mészáros | R. Wijers | R. Wijers | S. Campana | P. Romano | J. Cummings | C. Sarazin | S. Kobayashi | S. Patel | Y. Kaneko | B. Zhang | C. L. Sarazin | R. A. M. J. Wijers | J. R. Cummings | S. Patel | P. Meszaros | Y. Kaneko | M. Goad | A. King | L. Antonelli | B. Zhang | B. Zhang | B. Zhang | B. Zhang | M. B. Davies | J. Cummings | Shiho Kobayashi | P. Romano | J. Cummings | S. Kobayashi | P. O’Brien | A. King
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