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author 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.
author_facet 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.
author_sort Levan, A.
building Curtin Institutional Repository
collection Online Access
description 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.
first_indexed 2025-11-14T06:08:24Z
format Journal Article
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T06:08:24Z
publishDate 2011
publisher The American Association for the Advancement of Science
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-57172017-02-28T01:28:56Z An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy 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. 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. 2011 Journal Article http://hdl.handle.net/20.500.11937/5717 http://www.sciencemag.org/content/333/6039/199.full.pdf The American Association for the Advancement of Science restricted
spellingShingle 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.
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy
title An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy
title_full An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy
title_fullStr An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy
title_full_unstemmed An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy
title_short An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy
title_sort extremely luminous panchromatic outburst from the nucleus of a distant galaxy
url http://www.sciencemag.org/content/333/6039/199.full.pdf
http://hdl.handle.net/20.500.11937/5717