Fig. 4
X-ray light curve of GW Lib in the energy range 0.3–10 keV shown together with the optical V -band light curve. The optical fluxes are converted from 1d averaged V magnitudes from Kato et al. (2009) and the American Associationof Variable Star Observers (AAVSO) data base. The left (X-rays) and right (optical) axes have the same relative ranges.
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