This has been a fun few months for those interested in accretion-powered millisecond pulsars (and who isn't?) We've been observing HETE J1900.1-2455 for more than 3 years now, it has had by far the longest period of activity of any of the 8 known systems. Then, in August, IGR J00291+5934 went into outburst for the first time since it's December 2004 outburst. The X-ray flux faded shortly after, but the system unexpectedly returned to activity about a month later. To top it all off, the first-ever AMSP, SAX J1808.4-3658, also went into outburst in late September. Three AMSPs active at the same time is a terrific coincidence.

But there's more. Back in 2007 I made some predictions for the time of the next outburst for these two systems, based on the observed outbursts to date (see the table below). These predictions were remarkably accurate, with errors of 11 and 20 days (or 0.7 and 1.7%), for the two sources. For the record, I'm now prepared to make my predictions for the next outburst for each of these systems; for SAX J1808.4-3658 on 2012 May 15 (MJD 56062) and for IGR J00291+5934 a few months later on 2012 September 23 (MJD 56193). I hope to be able to report here how these new predictions hold up!
Table: Predictions of 2008 outburst times for two AMSPs (arXiv.org:0711.4420)

	Outburst time (MJD)
Source	predicted	actual	Error (d)
IGR J00291+5934	54680	54691	11
SAX J1808.4-3658	54710	54730	20

Labels: 2008, pulsars