Table 1: RXTE observations of Cep X-4 during 2002 June outburst. Luminosities are in the 2-10 keV range and are calculated using a distance of $3.8\pm 0.6$ kpc (Bonnet-Bidaud & Mouchet 1998).
Obs ID MJD Exposure Luminosity Period

70068-11- s $10^{36}~{\rm erg~s}^{-1}$ s

01-00 52439.9 800 1.40 66.41(0.05)

01-01 52442.1 816 1.06 66.36(0.04)

01-02 52444.7 880 0.87 66.25(0.04)

02-01 52450.1 1552 0.41 66.35(0.02)

02-000 52450.7 19600 0.35 66.30(0.01)

02-00 52451.0 1456 0.31 66.33(0.03)

02-02 52451.3 8432 0.32 66.30(0.01)

02-03 52451.7 7088 0.27 66.296(0.004)

**Table 1:** *RXTE* observations of Cep X-4 during 2002 June outburst. Luminosities are in the 2-10 keV range and are calculated using a distance of $3.8\pm 0.6$ kpc (Bonnet-Bidaud & Mouchet 1998).
Obs ID	MJD	Exposure	Luminosity	Period
70068-11-		s	$10^{36}~{\rm erg~s}^{-1}$	s
01-00	52439.9	800	1.40	66.41(0.05)
01-01	52442.1	816	1.06	66.36(0.04)
01-02	52444.7	880	0.87	66.25(0.04)
02-01	52450.1	1552	0.41	66.35(0.02)
02-000	52450.7	19600	0.35	66.30(0.01)
02-00	52451.0	1456	0.31	66.33(0.03)
02-02	52451.3	8432	0.32	66.30(0.01)
02-03	52451.7	7088	0.27	66.296(0.004)

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