Table 5. Impact of sampling frequency on period estimates (data sets with walking noise).
Shape1 | Method | 0.1 (3.0)2 | 1.0 (3.0)2 | 0.1 (5.0)2 | 1.0 (5.0)2 | 2.0 (5.0)2 | 2.0 (10)2 |
cos | EPR | 23.62 | 23.63 | 23.93 | 23.89 | 23.88 | 23.97 |
cos | MFF | 23.96 | 23.88 | 24.02 | 23.99 | 23.97 | 24.00 |
cos | NLLS | 23.89 | 23.84 | 23.98 | 23.96 | 23.96 | 24.00 |
cos | MESA | 23.81 | 23.87 | 23.95 | 23.94 | 23.95 | 23.99 |
cos | LSPR | 23.91 | 23.87 | 24.01 | 23.99 | 23.98 | 24.00 |
cos | SR | 24.2 | 24.25 | 24.11 | 24.09 | 24.07 | 24.01 |
asym | EPR | 24.54 | 24.48 | 24.06 | 24.1 | 24.09 | 24.08 |
asym | MFF | 24.16 | 24.05 | 24.09 | 24.06 | 24.03 | 24.09 |
asym | NLLS | 24.11 | 24.11 | 24.11 | 24.12 | 24.12 | 24.09 |
asym | MESA | 24.00 | 24.00 | 24.01 | 24.02 | 24.03 | 24.06 |
asym | LSPR | 24.65 | 24.55 | 24.28 | 24.28 | 24.24 | 24.13 |
asym | SR | 24.53 | 24.57 | 24.23 | 24.22 | 24.21 | 24.07 |
all | EPR | 24.02 | 23.99 | 24 | 23.98 | 23.98 | 24.01 |
all | MFF | 24.02 | 23.96 | 24.03 | 24.01 | 23.99 | 24.02 |
all | NLLS | 23.98 | 23.92 | 24.01 | 23.99 | 23.99 | 24.01 |
all | MESA | 23.89 | 23.91 | 23.96 | 23.95 | 23.96 | 23.99 |
all | LSPR | 24.22 | 24.14 | 24.1 | 24.09 | 24.07 | 24.03 |
all | SR | 24.40 | 24.40 | 24.16 | 24.14 | 24.13 | 24.01 |
Data sets with different time intervals and selected durations were analysed using all the methods and the mean period value is reported in the table (standard deviations are omitted for clarity). Data sets were created by adding walking noise of 80% of the original signal amplitude to the templates of different duration and time interval between points. The underlying period was 24.08 h for asym data and 24.00 h for the other signals. 1) The base shape of the signal: cosine (cos), pulse (pul); double pulse (dpl); shoulder (shl) and moderate asymmetry (asym), (all) represents aggregated results from all the sets. 2) the time interval (sampling frequency) in the data set and in brackets the data duration. See SI Table S5 for the full table.