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Table 1.

UBVRI time series of ω Cen and M 4 RRLs.

Name Flag (a) Band (b) HJD–2 400 000 Mag Err Dataset (c)
days mag mag
ωCen-V3 1 54705.4699 14.950 0.005 B19
ωCen-V3 1 50601.5756 14.767 0.022 B19
ωCen-V3 1 50601.5802 14.775 0.022 B19
ωCen-V3 1 50920.7741 15.335 0.017 B19
ωCen-V3 1 53795.8733 14.428 0.039 B19
ωCen-V3 1 53795.8858 14.487 0.065 B19
ωCen-V3 1 51368.4851 15.320 0.003 B19
ωCen-V3 1 51369.4884 15.339 0.003 B19
ωCen-V3 1 52443.4731 15.245 0.011 B19
ωCen-V3 1 52443.4773 15.223 0.011 B19

Notes. Optical 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, Col. 6 the photometric error and Col. 7 the dataset. Only the first ten entries are listed.

(a)

An asterisk in the second column indicates that the star was not used to derive the templates.

(b)

Photometric flag: “1” indicates data in the U band, “2” data in the B, “3” data in the V band, “4” data in the R band and “5” data in the I band.

(c)

Literature data flag: “B19” indicates data from our own photometry; “asa” indicates data from the ASAS-SN; “kal” indicates data from Kaluzny et al. (1997, 2004); “lub” indicates unpublished data by J.H. Lub; “stu” indicates data from Sturch (1978). The full table is available at the CDS.

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