Table 1: Properties of the accretion powered X-ray pulsars discussed in the text.

Source		 $P_{\rm s}$ $\nu_{\rm s}$ $\nu_{\rm QPO}$ $L_{\rm QPO}$ $L_{\rm tr}$ $x_{\rm QPO}^{\rm BFM}$ $x_{\rm QPO}^{\rm w}$ $x_{\rm QPO}^{\rm gl}$ Classificationa
        (band) (band)        
  s mHz mHz erg s-1 erg s-1        
        (keV) (keV)        

Her X-1 15,16,17		 1.24 806.5 8 $2.1\times10^{37}$ $2.1\times10^{37}$ 0.95-0.98 0.91-0.97 0.5 F
      43 (0.1-200) (0.1-200)        

4U 0115+63 9,10,18		 3.62 276.2 62 $8\times10^{37}$ $5\times10^{36}$ 0.56 0.61-0.71 0.23 F
        (0.1-200) (0.1-200)        

Cen X-3 13,14,19		 4.8 208.3 35 $ 1.0\times10^{38}$ $3.3\times10^{37}$ 0.89 0.82-0.92 0.36 F
        (0.12-100) (0.12-100)        

LMC X-4 11,12		 13.5 74.1 0.65-1.35 1039 $2\times10^{38}$ 0.97-0.98 0.76-0.88 0.31 F
        (2-25) (2-25)        

4U 1626-67 6,7,8		 7.66 130.6 40 $1.36\times10^{36}$ $1.7\times10^{36}$ 0.83 0.98-0.99 0.88 F/S
        (0.7-60) (0.7-60)        

EXO 2030+375 1,2		 42 23.8 213 $2\times10^{38}$ 1038 0.22 0.86-0.94 0.4 S
        (1-20) (1-20)        
  42 23.8 213 $2\times10^{38}$ $2.4\times10^{36}$ 0.22 0.43-0.56 0.14 S
        (1-20) (1-20)        

A 0535+262 3		 103 9.7 72 $4.3\times10^{37}$ $4.83\times10^{36}$ 0.24 0.69-0.82 0.26 S
        (20-100) (20-100)        

4U 1907+09 4,5		 440 2.3 55 $6.3\times10^{36}$ $2\times10^{36}$ 0.12 0.81-0.92 0.36 S
        (2-60) (1-15)        
a F = Fast rotator, S = Slow rotator.
References: (1) Parmar et al. (1989); (2) Angelini et al. (1989); (3) Finger et al. (1996); (4) Fritz et al. (2006); (5) in't Zand et al. (1998); (6) Chakrabarty et al. (1997); (7) Chakrabarty (1998); (8) Shinoda et al. (1990); (9) Tamura et al. (1992); (10) Campana et al. (2001); (11) Woo et al. (1996); (12) Moon & Eikenberry (2001a); (13) Howe et al. (1983); (14) Takeshima et al. (1991); (15) Dal Fiume et al. (1998); (16) Parmar et al. (1999); (17) Boroson et al. (2000); (18) Soong & Swank (1989); (19) Burderi et al. (2000).

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