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1RXH J082623.6–505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate

  • Authors: Kirill V. Sokolovsky, Jay Strader, Samuel J. Swihart, Elias Aydi, Arash Bahramian, Laura Chomiuk, Craig O. Heinke, Allison K. Hughes, Kwan-Lok Li, Raimundo Lopes de Oliveira, James C. A. Miller-Jones, Koji Mukai, David J. Sand, Laura Shishkovsky, Evangelia Tremou, Karina Voggel

Kirill V. Sokolovsky et al 2022 The Astrophysical Journal 934 .

  • Provider: AAS Journals

Caption: Figure 1.

XMM-Newton/EPIC 0.2–10 keV background-subtracted lightcurve of 1RXH J082623.6−505741. A minimal amount of the MOS 1/2 data was rejected due to background contamination, but the figure is much larger for the pn data, nearly 50%. Nonetheless, the vast majority of the potential 300 s bins for the pn lightcurve are usable, as they had at least a partial uncontaminated time interval. There is no systematic change in the count rate during the observation.

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