Table B.1.
Literature periods for sources not included in the Gavras et al. (2023) catalog. Variability types are either dubious, Semi-Regular variable (SR), long-period variable (LPV), Rotational variable (ROT), and RS Canum Venaticorum (RS CVn).
Gaia DR3 source id | Pph | Other ID | Lit. period | Variability type | Reference |
---|---|---|---|---|---|
(d) | (d) | ||||
1989111887224781056 | 36.89034 | ATO J346.0317+51.5494 | 77.013120 | dubious | (1) |
2037641061998679552 | 49.05138 | ATO J286.5005+28.5830 | 97.588819 | dubious | (1) |
629379460969722496 | 48.67723 | CSS J100138.5+204857 | 50.3620289 | (2) | |
1869696952997313664 | 52.81437 | ZTF J205411.65+353803.3 | 53.8513758 | SR | (3) |
ATO J313.5485+35.6342 | 106.784031 | LPV | (1) | ||
1756282633518972544 | 42.97533 | ASASSN-V J203640.72+133017.9 | 42.8644419 | ROT | (4) |
ATO J313.5485+35.6342 | 85.883021 | LPV | (1) | ||
2028753576416486912 | 63.55899 | ASASSN-V J195140.08+285735.1 | 63.1252006 | SR | (4) |
2230939471064416128 | 39.94571 | GCVS | 39.64 | RS CVn | (5) |
Notes. [1] ATLAS survey (Heinze et al. 2018); [2] Catalina Schmidt Survey (Drake et al. 2014); [3] Zwicky Transient Facility (Chen et al. 2020); [4] All-Sky Automated Survey for Supernovae (ASAS-SN; Jayasinghe et al. 2018); [5] Variable Star IndeX, from Kochanek et al. (2017).
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