Open Access
Table A.1
RRL stars rejected based on their light curves. Eclipsing binary types are denoted EA (detached), EB (semi-detached) and EW (contact)
| Gaia DR3 source_id | Comment |
|---|---|
| 51251471083601920 | Eclipsing (EB), P=2Psos |
| 201773650856861696 | Eclipsing (EB), P=2Psos |
| 87159184382553088 | Eclipsing (EB), P=2Psos |
| 182118845420393088 | Eclipsing (EB), P=2Psos |
| 412435405816698880 | G-band too sparse, P=2Psos |
| 412572810414744064 | Eclipsing (EB), P=2Psos |
| 248905041414230656 | Eclipsing (EB), P=2Psos |
| 258626781489990272 | Noisy, very low ampliture (0.2 in G) |
| 513743720002047488 | Noisy, double sequence |
| 668027908865948032 | Eclipsing (EW), P=2Psos |
| 3100435740214782080 | Too sparse, unlikely shape |
| 2208678999172871424 | Not an RRL. G/BP/RP well sampled too red, amplitude ratios inconsistent |
| 3108887445579879552 | Eclipsing (EB), P=2Psos |
| 3112279365934238720 | Probably Eclipsing (EA) |
| 3099365949760856448 | Eclipsing (EB/EW), P=2Psos |
| 3324366332775173760 | Probably Eclipsing (EA) |
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