Table 3
Pulsation periods of the sources.
| Source |  (days) |
 (days) |
Pw1 (days) | σW1 (days) | PW2 (days) | σW2 (days) | Pliterature (days) | Ref. | Padopted (days) | Comment |
|---|---|---|---|---|---|---|---|---|---|---|
| 1 - OH358.083+0.137 | … | … | … | … | … | … | … | Scatter, not periodic | ||
| 2 - OH358.162+0.490 | … | … | 1228 | 29 | 1272 | 60 | 1150, 1120 | 2, 3 | 1230 | Scatter in K |
| 3 - OH358.235+0.115 | … | … | … | … | … | … | 874 | 4 | 874 | Saturation in K and WISE |
| 4 - OH358.505+0.330 | … | … | … | … | … | … | … | Scatter, not periodic | ||
| 5 - OH359.140+1.137 | … | … | 1219 | 104 | 989 | 19 | … | 1000 | Very low-amplitude variability | |
| 6 - OH359.149−0.043 | … | … | … | … | … | … | … | Scatter. not periodic | ||
| 7 - OH359.220+0.163 | … | … | … | … | … | … | … | Scatter in K. too few datapoints in WISE | ||
| 8 - OH359.233−1.876 | … | … | … | … | … | … | … | Scatter in K. too few datapoints in WISE | ||
| 9 - OH359.467+1.029 | 604 | 3 | 604 | 1.3 | 605 | 2.4 | … | 605 | ||
| 10 - OH359.543−1.775 | … | … | … | … | … | … | 790 | 5 | Multi-periodic, non-Mira | |
| 11 - OH359.664+0.636 | … | 538 | 3.3 | 581 | 4.3 | … | 550 | Scatter in K | ||
| 12 - OH359.745−0.404 | 733 | 4 | 714 | 4.4 | 732 | 5.0 | 806, 766 | 1, 6 | 730 | |
| 13 - OH359.805+0.200 | 533 | 10 | 488 | 3.8 | 501 | 6.5 | … | 500 | ||
| 14 - OH359.826+0.153 | 501 | 3 | 483 | 2.1 | 489 | 4.3 | 493, 510 | 1, 6 | 500 | |
| 15 - OH359.902+0.061 | 586 | 13 | 611 | 3.4 | 588 | 5.1 | 558, 572, 550, 580 | 1, 7, 7, 8 | 590 | |
| 16 - OH0.173+0.211 | 512 | 4 | 510 | 5.5 | 516 | 6.8 | … | 512 | ||
| 17 - OH0.221+0.168 | 664 | 4 | 663 | 4.7 | 662 | 3.6 | 697 | 1 | 663 | |
| 18 - OH0.548−0.059 | … | … | … | … | … | … | … | Scatter, not periodic | ||
| 19 - OH0.739+0.411 | 577 | 10 | 557 | 2.8 | 602 | 2.8 | … | 570 | ||
| 20 - OH1.095−0.832 | … | … | … | … | … | … | … | Saturated | ||
| 21 - OH1.221+0.294 | 699 | 3 | 715 | 2.0 | 715 | 6.8 | … | 715 | ||
| 22 - OH1.628+0.617 | 921 | 43 | 827 | 6.5 | 839 | 8.0 | … | 830 |
Notes. Period with error in the Ks (2.15 µm) (Cols. 2, 3), W1 (3.4 µm) (Cols. 4, 5), and W2 (4.6 µm) (Cols. 6, 7) bands. Column (9): references for periods in the literature quoted in Col. (8): (1) Wood et al. (1998), (2) Le Bertre (1993), (3) Olivier et al. (2001), (4) present work, data from the Bochum Galactic Disk Survey (Hackstein et al. 2015) for source GDS_J1740541-302238, (5) present work, data from OGLE (Soszyński et al. 2013) for source OGLE-BLG-LPV-074942 classified as a semi-regular variable with principal period of 78.2 days, (6) Braga et al. (2019; also based on VVV data, but fewer data points than in the present study), (7) Glass et al. (2001; two periods from data in overlapping fields), (8) Matsunaga et al. (2009).
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