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    An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy

    Access Status
    Fulltext not available
    Authors
    Levan, A.
    Tanvir, N.
    Cenko, S.
    Perley, D.
    Wiersema, K.
    Bloom, J.
    Fruchter, A.
    de Ugarte Postigo, A.
    O’Brien, P.
    Butler, N.
    van der Horst, A.
    Leloudas, G.
    Morgan, A.
    Misra, K.
    Bower, G.
    Farihi, J.
    Tunnicliffe, R.
    Modjaz, M.
    Silverman, J.
    Hjorth, J.
    Thöne, C.
    Cucchiara, A.
    Castro Cerón, J.
    Castro-Tirado, A.
    Arnold, J.
    Bremer, M.
    Brodie, J.
    Carroll, T.
    Cooper, M.
    Curran, Peter
    Cutri, R.
    Ehle, J.
    Forbes, D.
    Fynbo, J.
    Gorosabel, J.
    Graham, J.
    Hoffman, D.
    Guziy, S.
    Jakobsson, P.
    Kamble, A.
    Kerr, T.
    Kasliwal, M.
    Kouveliotou, C.
    Kocevski, D.
    Law, N.
    Nugent, P.
    Ofek, E.
    Poznanski, D.
    Quimby, R.
    Rol, E.
    Romanowsky, A.
    Sánchez-Ramírez, R.
    Schulze, S.
    Singh, N.
    van Spaandonk, L.
    Starling, R.
    Strom, R.
    Tello, J.
    Vaduvescu, O.
    Wheatley, P.
    Wijers, R.
    Winters, J.
    Xu, D.
    Date
    2011
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Levan, A. and Tanvir, N. and Cenko, S. and Perley, D. and Wiersema, K. and Bloom, J. and Fruchter, A. et al. 2011. An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy. Science. 333: pp. 199-202.
    Source Title
    Science
    Additional URLs
    http://www.sciencemag.org/content/333/6039/199.full.pdf
    ISSN
    0036-8075
    URI
    http://hdl.handle.net/20.500.11937/5717
    Collection
    • Curtin Research Publications
    Abstract

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

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