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First Millimeter Flares Detected from ϵ Eridani with the Atacama Large Millimeter/submillimeter Array

  • Authors: Kiana Burton, Meredith A. MacGregor, Rachel A. Osten

Kiana Burton et al 2022 The Astrophysical Journal Letters 939 .

  • Provider: AAS Journals

Caption: Figure 2.

Light curves of the three major flaring events labeled E1, E2, and E3. Each light curve is centered on the flare peak, with the top x-axis indicating time relative to the flare peak in seconds. Each data point represents an individual ALMA integration (6 s in length, indicated by the x error bars). The shaded region in each plot indicates ± the rms noise level centered on a dashed line at 0 mJy.

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