text: 2009 Fermi Symposium, Washington, D.C., Nov. 2-5 
  
  12-25 keV band, where the ﬂux initially rose to about 
  240 mCrab (2009 Oct 25-28), suddenly dropped to 
  non-detectable on 2009 October 29-30, then rose again 
  during the period 2009 October 31 to November 2. As 
  of mid December 2009, the source remains in a high 
  intensity state. The light curve is shown for the pe- 
  riod MJD 54700-55200, again with 1-day resolution, 
  in Fig. 8. The ﬂuxes for XTE J1752-223 in Table 1 
  are given are for the interval of ﬂaring activity, TJD 
  55130-55180. 