In this paper, researchers conducted NuSTAR, Swift, and Chandra observations on the DQ Tau high-eccentricity binary system to confirm the presence of X-ray supe
This paper is available on arxiv under CC 4.0 license. Authors: Konstantin V. Getman, Department of Astronomy & Astrophysics, Pennsylvania State University; Agnes Kospal, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, E¨otv¨os Lor´and Research Network , MTA Centre of Excellence, Max Planck Institute for Astronomy, and ELTE E¨otv¨os Lor´and University, Institute of Physics; Nicole Arulanantham, Space Telescope Science Institute; Dmitry A.
Detection of Flares Figures 2a,b and 3a,b display the X-ray lightcurves and temporal evolution of the median energy for the X-ray events detected within the circular extraction regions depicted in Figure 1. In the shown lightcurve and median energy plots for NuSTAR, individual data points represent bins containing 30 X-ray events from the combined FPMA and FPMB data. Conversely, each point in the Swift-XRT and Chandra lightcurves and median energy plots corresponds to a single X-ray observation.
Detection of Flares Figures 2a,b and 3a,b display the X-ray lightcurves and temporal evolution of the median energy for the X-ray events detected within the circular extraction regions depicted in Figure 1. In the shown lightcurve and median energy plots for NuSTAR, individual data points represent bins containing 30 X-ray events from the combined FPMA and FPMB data. Conversely, each point in the Swift-XRT and Chandra lightcurves and median energy plots corresponds to a single X-ray observation.
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