Table 2
Comparison of the different observing runs on KUV 05134+2605.
| Run | Length | fR | Cov. | Noise | Points |
| (d) | (μHz) | (%) | (mmag) | ||
|
|
|||||
| 1988 | 5.99 | 1.9 | 7.5 | 1.2 | 1257 |
| 1992 | 1.16 | 9.9 | 34.0 | 1.0 | 3415 |
| 2000 Oct. | 5.11 | 2.3 | 8.2 | 0.8 | 3163 |
| WET2000 | 13.07 | 0.9 | 11.1 | 0.4 | 9516 |
| 2001 | 2.09 | 5.5 | 14.8 | 1.4 | 1147 |
| Konkoly2007 | 83.01 | 0.1 | 2.4 | 0.3 | 4936 |
| Konkoly2011 | 5.13 | 2.3 | 5.7 | 1.1 | 766 |
Notes. “Length” is the total time span of a run, fR denotes the corresponding Rayleigh frequency resolution, “Cov.” refers to the temporal coverage parameter, “Noise” is the average amplitude value in the 4050 − 5050 μHz frequency region, which is not affected by the star’s pulsation, and “Points” is the number of data points.
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