Pottschmidt, KatjaChernyakova, M.Zdziarski, A. A.Lubinski, P.Smith, D. M.Bezayiff, N.2023-10-062023-10-062005-12http://hdl.handle.net/11603/30027The Galactic Center black hole candidate (BHC) GRS 1758-258 has been observed extensively within INTEGRAL'S Galactic Center Deep Exposure program in 2003 and 2004, while also being monitored with RXTE. We present quasi-simultaneous PCA, ISGRI, and SPI spectra from four GCDE observation epochs. During the first epoch GRS 1758-258 displayed another of its rare dim soft states like the one observed in 2001. In the recently emerging picture of the hardness-intensity evolution of black hole transient outbursts in which hard and soft states are observed to occur in a large overlapping range of luminosities (hysteresis), the dim soft state is not peculiar.2 pagesen-USThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.Text