Fig. 1
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Light curve of EX Lupi spanning the last ~130 yr. The photometry is a combination of Visible and V magnitudes taken from DASCH (red markers) and AAVSO (blue markers). It shows three large outbursts in 1944 (see Appendix A), 1955 (Herbig 1977) and 2008 (Jones 2008), multiple bursts reported by McLaughlin (1946), Bateson et al. (1991), Herbig et al. (2001), Herbig (2007) and the one presented in this work (see Fig. 2).
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