XTE J1550-564 brightening again According to IAUCs 7575, the southern black hole X-ray transient (X-ray nova) XTE J1550-564 is brightening again. The source has brigtened V=18.3 on Jan. 28-30 (R magnitudes are typically 1 mag brighter). The source was first observed in outburst in 1998 September (IAUC 7008), whose optical counterpart (V=16) was immediately discovered at 15h 50m 58s.78, -56o 28' 35".0 (J2000.0, IAUC 7009). Among VSNET members, Gordon Garradd observed the source for several nights. The present renewed activity may or may not resemble "mini-outbursts" notably observed in GRO J0422+32 (=V518 Per). Another outburst was observed in 2000 April (IAUC 7399, 7400). The object would be well observed using a small telescope with a CCD. Sequence information: see vsnet-alert 4607, 4608 Regards, VSNET Collaboration team (PS. Among the transients in 1998, the object still lacks the GCVS designation)