The distribution of kHz QPO frequencies in Sco X-1
  The frequencies of kHz Quasi-Periodic Oscillations in the bright Low-Mass X-ray Binary Sco X-1 have been reported to appear preferentially in a 3:2 ratio. We show that a proper statistical analysis of those RXTE data upon which the claim is based indicated a 2.4 sigma deviation from a constant distribution in ratios. The analysis of a much larger RXTE/PCA dataset shows that there is no sharp concentration around a 3:2 ratio, but that the ratios are broadly distributed over the range 820-1150 Hz. 
Tomaso Belloni (INAF - Oss. Astr. Brera, Italy), Mariano Mendez (SRON,   Utrecht, the Netherlands), Jeroen Homan (MIT, USA)