text: GRS 1915+105 (Fig. 5) is a LMXB with the com- 
  pact object being a massive black hole. Evidence for 
  emission above 100 keV has been seen previously [12] 
  with BATSE. The GBM light curve integrated over 
  490 days shows signiﬁcant emission above 100 keV. 
  
  1E 1740-29 (Fig. 6) is a LMXB very near the 
  Galactic Center. It is a microquasar, and spends most 
  Integral observa- 
  of its time in the low/hard state. 
  tions indicate the presence of a power law tail above 
  200 keV [13]. The present GBM results are consis- 
  tent with this high energy emission. In the future, we 
  
  eConf C091122 