4U 1630-472: The peak X-ray flux was obtained from the 2003 outburst ( Tomsick2005 ) , the brightest one detected so far. It has shown quasi-periodic outburst with recurrence times of ∼600-700 d and durations of 100-200 d ( Kuulkers1997 ). The K-band magnitude was not transformed into AB system.
This research has made use of NASA's Astrophysics Data System (ADS) and the SIMBAD database operated at CDS (Strasbourg, France)
Please acknowledge the use of this catalogue in any published work you derive from it.