Swift observations of the SFXT SAX J1818.6-1703 in outburst
P. Romano (1), L. Sidoli (2), P. Esposito (2), V. la Parola (1), J.A., Kennea (3), H.A. Krimm (4,5), M.M. Chester (3), A. Bazzano (6), D.N. Burrows, (3), N. Gehrels (4) ((1) Inaf-Iasf Palermo, (2) Inaf-Iasf Milano, (3) Psu,, (4) NASA/GSFC, (5) Usra, (6) Inaf-Iasf Roma)

TL;DR
This paper reports Swift telescope observations of the SFXT SAX J1818.6-1703 during its recent outburst, providing spectroscopic and timing analysis that confirm its classification within the supergiant fast X-ray transient class.
Contribution
First detailed broad-band spectroscopic and timing analysis of SAX J1818.6-1703 during an outburst, confirming its membership in the SFXT class.
Findings
Outburst duration and spectral properties resemble those of XTE J1739-302.
Broad-band spectral models support classification as an SFXT.
Light curve analysis spans over two weeks of observations.
Abstract
We present the Swift observations of the supergiant fast X-ray transient (SFXT) SAX J1818.6-1703 collected during the most recent outburst, which occurred on May 6 2009. In particular, we present broad-band spectroscopic and timing analysis as well as a Swift/XRT light curve that spans more than two weeks of observations. The broad-band spectral models and length of the outburst resemble those of the prototype of the SFXT class, XTE J1739-302, further confirming SAX J1818.6-1703 as a member of this class.
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