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• W2773809501 abstract "We present Large Binocular Telescope difference imaging data for the final years of four Type II-P/L supernovae progenitors. For all four, we find no significant evidence for stochastic or steady variability in the U, B, V, or R bands. Our limits constrain variability to no more than roughly 5–10per cent of the expected R-band luminosities of the progenitors. These limits are comparable to the observed variability of red supergiants in the Magellanic Clouds. Based on these four events, the probability of a Type II-P/L progenitor having an extended outburst after Oxygen ignition is |$lt 37{{ rm per cent}}$| at 90 per cent confidence. Our observations cannot exclude short outbursts in which the progenitor returns to within |${sim }10{{ rm per cent}}$| of its quiescent flux on the time-scale of months with no dust formation." @default.
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• W2773809501 date "2018-07-23" @default.
• W2773809501 modified "2023-10-18" @default.
• W2773809501 title "The quiescent progenitors of four Type II-P/L supernovae" @default.
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• W2773809501 doi "https://doi.org/10.1093/mnras/sty1966" @default.
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