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An extremely luminous panchromatic outburst from the nucleus of a distant galaxy

Levan, AJ, Tanvir, NR, Cenko, SB, Perley, DA, Wiersema, K, Bloom, JS, Fruchter, AS, De Ugarte Postigo, A, O'Brien, PT, Butler, N, Van Der Horst, AJ, Leloudas, G, Morgan, AN, Misra, K, Bower, GC, Farihi, J, Tunnicliffe, RL, Modjaz, M, Silverman, JM, Hjorth, J , Thöne, C, Cucchiara, A, Castro Cerón, JM, Castro-Tirado, AJ, Arnold, JA, Bremer, M, Brodie, JP, Carroll, T, Cooper, MC, Curran, PA, Cutri, RM, Ehle, J, Forbes, D, Fynbo, J, Gorosabel, J, Graham, J, Hoffman, DI, Guziy, S, Jakobsson, P, Kamble, A, Kerr, T, Kasliwal, MM, Kouveliotou, C, Kocevski, D, Law, NM, Nugent, PE, Ofek, EO, Poznanski, D, Quimby, RM, Rol, E, Romanowsky, AJ, Sánchez-Ramírez, R, Schulze, S, Singh, N, Van Spaandonk, L, Starling, RLC, Strom, RG, Tello, JC, Vaduvescu, O, Wheatley, PJ, Wijers, RAMJ, Winters, JM and Xu, D (2011) An extremely luminous panchromatic outburst from the nucleus of a distant galaxy. Science, 333 (6039). pp. 199-202. ISSN 0036-8075

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Abstract

Variable x-ray and γ-ray emission is characteristic of the most extreme physical processes in the universe. We present multiwavelength observations of a unique γ-ray-selected transient detected by the Swift satellite, accompanied by bright emission across the electromagnetic spectrum, and whose properties are unlike any previously observed source. We pinpoint the event to the center of a small, star-forming galaxy at redshift z = 0.3534. Its high-energy emission has lasted much longer than any γ-ray burst, whereas its peak luminosity was ∼100 times higher than bright active galactic nuclei. The association of the outburst with the center of its host galaxy suggests that this phenomenon has its origin in a rare mechanism involving the massive black hole in the nucleus of that galaxy.

Item Type: Article
Additional Information: This is the accepted version of the following article: Levan et al. An extremely luminous panchromatic outburst from the nucleus of a distant galaxy. Science; Vol:333, Is: 6039;pp199-202, which has been published in final form at http://dx.doi.org/10.1126/science.1207143
Uncontrolled Keywords: MD Multidisciplinary
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: American Association for the Advancement of Science
Date Deposited: 25 May 2017 08:50
Last Modified: 04 Sep 2021 11:30
DOI or ID number: 10.1126/science.1207143
URI: https://researchonline.ljmu.ac.uk/id/eprint/6568
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