Overview of an extensive multi-wavelength study of GX 339−4 during the 2010 outburst (Corrigendum)
M. Cadolle Bel1, J. Rodriguez2, P. D’Avanzo3, D. M. Russell4, J. Tomsick5, S. Corbel2, F. W. Lewis6, F. Rahoui7, M. Buxton8, P. Goldoni9 and E. Kuulkers1
1 ESAC, ISOC, Villañueva de la Cañada, Madrid, Spain
e-mail: Marion.Cadolle@sciops.esa.int
2 Laboratoire AIM, UMR 7158, CEA/DSM – CNRS – Université Paris Diderot, IRFU/SAp, Gif-sur-Yvette, France
3 INAF, Osservatorio Astronomico di Brera, 23807 Merate, Italy
4 University of Amsterdam (Anton Pannekoek Institute), The Netherlands
5 SSL/California University, Berkeley, USA
6 Faulkes Telescope Project, University of Glamorgan, Wales, UK
7 Astronomy Department, Harvard University & Harvard-Smithsonian Center for Astrophysics, Cambridge, USA
8 Astronomy Department, Yale University, USA
9 Laboratoire APC, UMR 7164, CEA/DSM – CNRS – Université Paris Diderot, IRFU/SAp, Paris, France
This article has no abstract.
Key words: black hole physics / stars: individual: GX 339 / 4 / X-rays: binaries / gamma rays: general / infrared: general / errata, addenda
© ESO, 2012

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