J. Wilms (1), M.A. Nowak (2), K. Pottschmidt (3,4), R. Staubert (1), E. Kendziorra (1), T. Gleissner (1) and P. Predehl (3)
(1) Institut für Astronomie und Astrophysik, Astronomie, Universität
Tübingen, Sand 1, D-72076 Tübingen, Germany
(2) MIT, 77 Massachusetts Ave., Cambridge MA02139, USA
(3) MPE, Postfach 1312, 85741 Garching, Germany
(4) ISDC, 16 Ch. d'Ecogia, 1290 Versoix, Switzerland
To appear in: Proceedings of the 4th Microquasar Workshop, eds. Ph Durouchoux, Y. Fuchs and J. Rodriguez, published by the Center for Space Physics: Kolkata
Abstract. We present first results of the analysis of XMM-Newton observations of the black hole candidates GX 339-4 and LMC X-1. The flux level and spectral shape of GX 339-4 during its recent "off state" were comparable with earlier BeppoSAX observations. LMC X-1 was observed during its usual soft state.Key words: -
Paper (135k gzip'ed Postscript including figures)
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