  We present a 2 - 10 keV ASCA observation of the field around the soft gamma
repeater SGR1627-41. A quiescent X-ray source was detected in this observation
whose position was consistent both with that of a recently discovered BeppoSAX
X-ray source and with the Interplanetary Network localization for this SGR. In
2 - 10 keV X-rays, the spectrum of the X-ray source may be fit equally well by
a power law, blackbody, or bremsstrahlung function, with unabsorbed flux ~5 x
10^-12 erg cm^-2 s^-1. We do not confirm a continuation of a fading trend in
the flux, and we find no evidence for periodicity, both noted in the earlier
BeppoSAXobservations.
