Suzaku Observation of the New Soft Gamma Repeater Sgr 0501+4516 in Outburst

We present the first Suzaku observation of the new Soft Gamma Repeater SGR0501+4516, performed on 2008 August 26, four days after the onset of bursting activity of this new member of the magnetar family. The soft X-ray persistent emission was detected with the X-ray Imaging Spectrometer (XIS) at a 0.5–10 keV flux of 3.8 × 10 erg scm, with a spectrum well fitted by an absorbed blackbody plus power-law model. The source pulsation was confirmed at a period of 5.762072 ± 0.000002 s, and 32 X-ray bursts were detected by the XIS, four of which were also detected at higher energies by the Hard X-ray Detector (HXD). The strongest burst, which occurred at 03:16:16.9 (UTC), was so bright that it caused instrumental saturation, but its precursor phase, lasting for about 200ms, was detected successfully over the 0.5–200 keV range, with a fluence of ∼ 2.1 × 10 erg cm and a peak intensity of about 89 Crab. The entire burst fluence is estimated to be ∼ 50 times higher. The precursor spectrum was very hard, and well modeled by a combination of two blackbodies. We discuss the bursting activity and X/γ-ray properties of this newly discovered Soft Gamma Repeater in comparison with other members of the class. Subject headings: pulsar: individual (SGR 0501+4516) — stars: magnetic fields — X-rays: stars