text: source while it is in the hard state, with longer obser- 
  vations potentially verifying signiﬁcant emission above 
  300 keV. 
  will use the GBM CSPEC data with their ﬁner energy 
  bins to obtain a ﬁt to the spectrum and compare the 
  power law index to that measured by Integral. 
  
  SWIFT J1753.5-0127 (Fig. 7) is a LMXB with 
  the compact object likely being a black hole. Swift 
  discovered this source when it observed a large ﬂare 
  in July of 2005. The source did not return to qui- 
  escence but settled into a low intensity hard state 
  [14]. BATSE occultation measurements from 1991- 
  2000 showed no signiﬁcant emission from this source 
  above 25 keV [15]. The GBM results show that this 
  source is still in a hard state, with signiﬁcant emis- 
  sion above 100 keV. We will continue to monitor this 
  
  B. Transient Source 
  
  The new transient black hole candidate XTE 
  J1752-223 rose from undetectable on 2009 October 
  24 to 511 ± 50 mCrab (12 - 25 keV), 570 ± 70 mCrab 
  (25 - 50 keV), 970 ± 100 mCrab (50 - 100 keV), and 
  330 ± 100 mCrab (100 - 300 keV) on 2009 November 
  2 [2, 16]. The light curve is variable, especially in the 