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Table 2

Phase-averaged cyclotron line energies Ecyc and maximum fluxes reproduced from Staubert et al. (2007) (1) and from the spectral re-analysis of this work (2).

35 d cycle Ecyc(1) [keV] max. flux (2–10 keV) Ecyc(2) [keV] max. flux (3.5–60 keV)2
number1 ASM [cts   s-1] [10-9   erg   cm-2   s-1]
(Staubert et al. 2007) (Staubert et al. 2007) (this work) (this work)

257 41.12 ± 0.55 7.37 ± 0.34 40.61 ± 0.34 7.99 ± 0.45
269 40.62 ± 0.49 7.49 ± 0.73 40.45 ± 0.41 8.02 ± 0.46
303 40.07 ± 0.31 6.04 ± 0.47 39.81 ± 0.24 7.27 ± 0.41
304 39.05 ± 0.55 5.72 ± 0.34 38.72 ± 0.31 7.14 ± 0.40
307 39.93 ± 0.63 7.15 ± 0.50 39.78 ± 0.49 8.26 ± 0.47
308 39.73 ± 0.52 6.93 ± 0.20 40.04 ± 0.33 8.18 ± 0.46
320 40.01 ± 0.29 7.19 ± 0.26 39.94 ± 0.29 9.55 ± 0.36
323 40.51 ± 0.13 7.64 ± 0.30 40.16 ± 0.11 9.37 ± 0.44
324 40.60 ± 0.41 7.55 ± 0.34 40.37 ± 0.35 9.16 ± 0.52
343 38.51 ± 0.51 4.50 ± 0.24 38.26 ± 0.43 7.05 ± 0.40
351 38.95 ± 0.52 5.12 ± 0.37 39.28 ± 0.60 6.61 ± 0.38

Notes. 

(1)

Note that for 35 d cycle numbers 303 and larger the corresponding numbers in Staubert et al. (2007) are larger by 1. This reflects the observation that there must have been an extra cycle during the long anomalous low before cycle 303. However, using the numbers as given here allows to use them in an ephemeris for a rough prediction of the 35 d turn-ons using a mean period of 35.88 d. We do not doubt the physical reality of the extra cycle found by Staubert et al. (2007).

(2)

The flux in Col. 5 represents the 35 d maximum flux in the 3.5–60 keV range (see text).

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