Table 2.
JHKs time series of ω Cen, M 4 and BW RRLs.
| Name | Flag (a) | Band (b) | HJD–2 400 000 | Mag | Err |
|---|---|---|---|---|---|
| days | mag | mag | |||
| ωCen-V3 | 1 | 55341.5764 | 13.137 | 0.006 | |
| ωCen-V3 | 1 | 55341.5878 | 13.147 | 0.007 | |
| ωCen-V3 | 1 | 55341.6006 | 13.175 | 0.004 | |
| ωCen-V3 | 1 | 55341.6074 | 13.179 | 0.013 | |
| ωCen-V3 | 1 | 51946.8638 | 13.053 | 0.013 | |
| ωCen-V3 | 1 | 51948.7440 | 13.154 | 0.012 | |
| ωCen-V3 | 1 | 51948.8136 | 13.170 | 0.008 | |
| ωCen-V3 | 1 | 52308.7494 | 13.075 | 0.013 | |
| ωCen-V3 | 1 | 52308.8255 | 13.117 | 0.016 | |
| ωCen-V3 | 1 | 52308.8674 | 13.145 | 0.011 |
Notes. NIR time series for cluster RRLs. Column 1 gives the name, Col. 2 is a flag which marks the variables that were used to build the templates, Col. 3 gives the filter, Col. 4 the Heliocentric Julian Day of the observation, Col. 5 the measured magnitude and Col. 6 the photometric error. Only the first ten entries are listed.
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