XMM-Newton study of the Sculptor dwarf spheroidal galaxy
Sara Saeedi, Manami Sasaki

TL;DR
This study used XMM-Newton observations to classify X-ray sources in the Sculptor dwarf spheroidal galaxy, identifying various background and member sources, including potential X-ray binaries and symbiotic stars, with no significant long-term variability or pulsations detected.
Contribution
It provides the first detailed classification of X-ray sources in Sculptor dSph, distinguishing between background objects and galaxy members using multi-wavelength analysis.
Findings
Identified 43 background AGNs and galaxy candidates.
Detected 4 symbiotic star candidates and 3 quiescent low-mass X-ray binaries.
Found no significant long-term variability or pulsations in the sources.
Abstract
We analysed observations with XMM-Newton in the field of the Sculptor dwarf spheroidal galaxy (dSph). The aim of the study was the classification of X-ray binaries and accreting white dwarfs, which belong to the Sculptor dSph. Using different methods of X-ray timing and spectral analyses, together with an extensive multi-wavelength study of the optical and infrared counterparts of the X-ray sources, we classified the sources detected with XMM-Newton in the field of Sculptor dSph. The long term variability of the sources has been studied over two \xmm\, observations. None of the members of Sculptor dSph show a significant long-term variability over these two observations. We also searched for periodicity and pulsation using the Lomb-Scargle and Rayleigh's Z_n^2 techniques. No signal of pulsation or periodicity have been found for the X-ray sources. The results show the presence of a…
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.
