INITIAL RESULTS FROM NuSTAR OBSERVATIONS OF THE NORMA ARM

Results are presented for an initial survey of the Norma Arm gathered with the focusing hard X-Ray Telescope NuSTAR. The survey covers 0.2 deg2 of sky area in the 3–79 keV range with a minimum and maximum raw depth of 15 ks and 135 ks, respectively. Besides a bright black-hole X-ray binary in outburst (4U 1630−47) and a new X-ray transient (NuSTAR J163433−473841), NuSTAR locates three sources from the Chandra survey of this region whose spectra are extended above 10 keV for the first time: CXOU J163329.5−473332, CXOU J163350.9−474638, and CXOU J163355.1−473804. Imaging, timing, and spectral data from a broad X-ray range (0.3–79 keV) are analyzed and interpreted with the aim of classifying these objects. CXOU J163329.5−473332 is either a cataclysmic variable or a faint low-mass X-ray binary. CXOU J163350.9−474638 varies in intensity on year-long timescales, and with no multi-wavelength counterpart, it could be a distant X-ray binary or possibly a magnetar. CXOU J163355.1−473804 features a helium-like iron line at 6.7 keV and is classified as a nearby cataclysmic variable. Additional surveys are planned for the Norma Arm and Galactic Center, and those NuSTAR observations will benefit from the lessons learned during this pilot study.