Table 3.
Ks-band time series of our candidate variables.
| Name | HJD–2 400 000 | Mag | Err |
|---|---|---|---|
| days | mag | mag | |
| b333_59_98743 | 55844.02155 | 14.704 | 0.043 |
| b333_59_98743 | 55423.14904 | 14.607 | 0.040 |
| b333_59_98743 | 55777.13660 | 14.865 | 0.054 |
| b333_59_98743 | 55778.19837 | 14.627 | 0.032 |
| b333_59_98743 | 55794.12621 | 14.657 | 0.047 |
| b333_59_98743 | 55806.15221 | 14.674 | 0.046 |
| b333_59_98743 | 55820.10395 | 14.705 | 0.045 |
| b333_59_98743 | 55830.02354 | 14.807 | 0.044 |
| b333_59_98743 | 55849.02315 | 14.518 | 0.036 |
| b333_59_98743 | 55987.37349 | 14.730 | 0.052 |
Notes. Column 1 gives the name, Col. 2 the heliocentric Julian day of the observation, Col. 3 the measured magnitude and Col. 4 the photometric error. We note that the light curves of Miras – except those in common with M09 – are not within this table and will be published in Nikzat et al. (in prep.). Only the first ten entries are listed. The full table is provided at the CDS.
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