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Table 1

Time-series photometry for all known and new variables in the field of view covered in Terzan 5.

Cluster var Filter HJD Mstd Mins σm fref σreſ fdiff σdiff p
ID (d) (mag) (mag) (mag) (ADU s−1) (ADU s−1) (ADU s−1) (ADU s−1)
Terzan5 V3 I 2456 847.71238 18.274 9.569 0.017 1321.348 329.766 +001166.327 161.418 7.0252
Terzan5 V3 I 2456 848.49854 18.421 9.716 0.032 1321.348 329.766 -000190.850 331.537 8.6296
Terzan5 V14 I 2456847.71238 14.633 5.928 0.001 40 810.543 333.083 +012128.637 379.316 7.0252
Terzan5 V14 I 2456848.49854 14.639 5.933 0.002 40810.543 333.083 +013131.433 548.535 8.6296
Terzan5 V15 I 2456847.71238 14.916 6.211 0.002 33 569.503 339.078 -005486.698 360.373 7.0252
Terzan5 V15 I 2456848.49854 14.914 6.208 0.002 33 569.503 339.078 -006093.916 532.514 8.6296

Notes. The standard Mstd and instrumental Mins magnitudes are listed in Cols. 5 and 6, respectively, corresponding to the cluster, variable star, filter, and epoch (UTC) of mid-exposure listed in Cols. 1–4, respectively. The uncertainty in Mins is listed in Col. 7, which also corresponds to the uncertainty in Mstd. For completeness, we also list the quantities ƒref, ƒdiff, and p from Eq. (2) in Cols. 8, 10, and 12, along with the uncertainties σref and σdif in Cols. 9 and 11, respectively. This is an extract from the full table, which is available at the CDS.

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