data suggest a few points at $L_X\sim10^{38}$ ergs/s from NGC 6440, suggesting X-ray bursts, their 6-sigma maximum significance is matched by similar points from black hole candidates in the Galactic Center. Thus we cannot be assured of their reality.) Scans in late May 2009 showed evidence for an increased countrate from NGC 6440 (see 3rd red line in Fig. \[fig:lcurve\]). An outburst was confirmed by  observations in early June (see below). No further activity was observed until a scan showed a 5-sigma detection on July 28, 2009, near the beginning of the  observation. A pointed  observation on July 30 showed a significant decline from the  and bulge scan fluxes (details below). Later bulge scans (on Aug. 1st & 2nd) were consistent with a decay below the PCA’s (background-limited, due to its non-imaging nature) sensitivity (Fig. \[fig:lcurve\]).

A third bulge scan peak on August 29, 2009 triggered a pointed observation Aug. 30, which discovered millisecond pulsations from NGC 6440 X-2 with a frequency of 205 Hz [@Altamirano09]. Further  observations starting on Sept. 1st found fluxes returning to quiescence. Upon identifying a fourth outburst with /XRT on Oct. 1st, 2009, a pointed  observation on Oct. 2nd detected NGC 6440 X-2 near the 