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We present a detailed timing and spectral analysis of the Be X-ray binarySWJ2000.6+3210 discovered by the BAT Galactic plane survey. Two Suzakuobservations of the source made at six months interval, reveal pulsations at ~890s for both observations with a much weaker pulse fraction in the second one.Pulsations are clearly seen in the energy band of 0.3-10 keV of XIS for bothobservations and at high energies up to 40 keV for the second observation. Thebroad band X-ray spectrum is consistent with a powerlaw and high energy cutoffmodel along with a hot blackbody component. No change in spectral parameters isdetected between the observations. We have also analyzed several shortobservations of the source with Swift/XRT and detected only a few percentvariation in flux around a mean value of 3:5 *10^{-11} erg cm^{-2} s^{-1}. Theresults indicates that SWJ2000.6+3210 is a member of persistent Be X-raybinaries which have the same broad characteristics as this source.

Revisiting SWJ2000.6+3210 : A persistent Be X-ray pulsar ?