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Fig. 22.

image

Top: amplitude variations of the ten δ Scuti frequencies of HD 184465 with signal to noise ratios greater than four from 2008 to 2011, with one point per winter. Bottom: amplitude variations of three frequencies with two time intervals for each of the 2008, 2009, and 2010 winters and six 30-day intervals for the 2011 winter. The 3σ uncertainties are shown for the main frequency and are the same for all frequencies.

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