V381 Nor = XTE J1550-564 outburst, slightly faded The fading rate may be slightly larger than those of typical (classical) black hole X-ray transients. YYYYMMDD(UT) mag observer 20030328.910 170CR (Berto Monard) 20030330.010 169CR (Berto Monard) 20030424.012 177CR (Berto Monard)
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