Table 3.
Variability measures for the long-term NED02 X-ray light curves for the Chandra exposures, quantifying the variability size and timing.
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MDDE (b) | MR/MRE (c) | TMDDE (d) | WMEAN (e) | EMFU/EMFD (f) | TEMFU/TEMFD (g) | |
---|---|---|---|---|---|---|---|
All four ObsIDs | 15.662/ | 9.129 | 11.400/ | 708.51 | 0.132 | 5.588/ | 709.49/ |
∼0 | 14.021 | 2.033 | 4.24 | ||||
4187 omitted | 2.420/ | 5.515 | 2.553/ | 4.24 | 0.183 | 1.766/ | 0.79/ |
5.327 × 10−12 | 0.070 | 2.033 | 4.24 | ||||
ET2U/ET2D (h) | ET10U/ET10D (i) | ZWW(j) | |||||
All 4 ObsIDs | 708.49/ | n.a./ | −10.768 | ||||
4.24 | n.a. | ||||||
4187 Omitted | n.a/ | n.a./ | −12.658 | ||||
4.24 | n.a |
Notes.
Reduced about the error-weighted mean count rate, and the corresponding p-value. p-values < 0.0027 are deemed significant (i.e., nonvariability is improbable) at a 3σ level.
Shortest time interval (in days) for a count rate increase (ET2U) or decrease (ET2D) by a factor > 2, i.e., where . If no such interval exists, we report as n.a.
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