Detection of a Rare Supersoft Outburst Event during a Suzaku Observation of 1E0102.2-7219
D. Takei, M. Tsujimoto, S. Kitamoto, M. Morii, K. Ebisawa, Y. Maeda,, and E. D. Miller

TL;DR
This paper reports the discovery of a rare, transient supersoft X-ray source in the Small Magellanic Cloud during a Suzaku observation, characterized by a brief, bright outburst with spectral features typical of supersoft sources.
Contribution
First detection of a transient supersoft X-ray source in the SMC using Suzaku, providing insights into the properties and behavior of such rare objects.
Findings
Detected a transient supersoft X-ray source with a brief outburst.
Spectral analysis shows a blackbody temperature of ~72 eV and an absorption edge at ~0.74 keV.
The source's luminosity and size are consistent with supersoft sources in the SMC.
Abstract
We report the detection of a transient X-ray source toward the Small Magellanic Cloud (SMC) using the X-ray Imaging Spectrometer (XIS) onboard the Suzaku telescope. The source was detected at the edge of the XIS image during a routine observation of the calibration source 1E 0102.2-7219, a supernova remnant in the SMC. We constrained the source position using ray-tracing simulations. No such transient source was found at the position in the other Suzaku observations nor in all the available archived images of other X-ray missions for the last ~28 years. The XIS spectrum can be explained by a single blackbody with a temperature of ~72 eV, and an interstellar extinction of ~4.9x10^{20} H atoms cm^{-2} consistent with the value to the SMC. An additional absorption edge at ~0.74 keV was also confirmed, which is presumably due to the absorption by helium-like oxygen ions. Assuming that the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
