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Table B.3.

Amplitude of the ten δ Scuti frequencies with signal to noise ratios greater than four found in the Fourier spectrum of HD 184465 for each winter and for the four winters together.

Frequency (d−1) 2008 2009 2010 2011 All
9.671458 (12) 0.86 (32) 2.24 (24) 3.60 (19) 5.98 (14) 3.94 (10)
6.465094 (56) 1.33 (32) 0.90 (24) 0.93 (19) 0.67 (14) 0.85 (10)
8.691272 (64) 0.26 (32) 0.34 (24) 0.28 (19) 1.41 (14) 0.74 (10)
4.934047 (69) 0.79 (32) 0.57 (24) 0.72 (19) 0.69 (14) 0.68 (10)
3.785687 (87) 0.36 (32) 0.38 (24) 0.63 (19) 0.61 (14) 0.55 (10)
14.20371 (12) 0.07 (32) 0.06 (24) 0.19 (19) 0.74 (14) 0.40 (10)
4.35554 (13) 0.24 (32) 0.40 (24) 0.36 (19) 0.53 (14) 0.37 (10)
7.70589 (18) 0.26 (32) 0.38 (24) 0.38 (19) 0.18 (14) 0.26 (10)
10.03363 (25) 0.39 (32) 0.29 (24) 0.19 (19) 0.32 (14) 0.19 (10)
11.82126 (26) 0.19 (32) 0.27 (24) 0.10 (19) 0.22 (14) 0.19 (10)

Notes. Numbers in parentheses indicate the 3σ uncertainties on the last two digits. The amplitudes are in mmag.

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