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. 2018 Sep 10;9:1276. doi: 10.3389/fphys.2018.01276

Table 1.

Free-running activity rhythms in DD.

Genotype n Period (h) ± SEM Power ± SEM R (%)
w1118 62 24.2 ± 0.1 151.6 ± 6.6 90.3
CCHa1SK8 32 24.2 ± 0.1 178.3 ± 8.5 100
CCHa1MI09190 31 23.7 ± 0.1∗∗ 123.9 ± 7.8 90.3
tim/+ 32 24.6 ± 0.1 214.5 ± 8.6 100
clk856/+ 31 24.1 ± 0.1 143.7 ± 8.6 83.9
+/CCHa1RNAi 32 24.5 ± 0.1 211.4 ± 8.7 96.9
+/CCHa1-RRNAi 32 24.5 ± 0.1 153.5 ± 6.7 96.9
tim > CCHa1RNAi 32 24.2 ± 0.1 175.8 ± 11.7 96.9
clk856 > CCHa1RNAi 63 23.8 ± 0.1∗∗ 151.4 ± 5.7 95.2
tim > CCHa1-RRNAi 32 23.5 ± 0.1∗∗ 173.4 ± 9.2 96.9

DD, constant darkness; CCHa1, CCHamide1; SEM, standard error of the mean. The free-running period, power, and rhythmicity (R) was determined from data of days 1–10 of DD using χ2-periodogram analysis. CCHa1 mutants and RNAi strains were compared with the corresponding control lines, e.g., UAS or Gal4 control lines. If period or power was significantly different from both of the corresponding control lines, it was designated as statistically significant. One-way ANOVA with Tukey’s multiple comparison test was used after testing for the normal distribution of data using the Kolmogorov–Smirnov test; p < 0.05, ∗∗p < 0.01.