Table A.2
Twenty RR Lyrae stars identified in UMi by N88 that are included in the Gaia DR3 vari_rrlyrae table or are classified as ‘RR’ in the DR3 vari_classifier_result table.
| Name | source_id | P | Type | P | Type | P | Type |
|---|---|---|---|---|---|---|---|
| N88 | Gaia DR3 | N88 (days) | N88 | vari_rrlyrae table (days) | vari_rrlyrae table | this work (days) | this work |
| V3 | 1645474367067330048 | 0.383 | c | 0.27660 | c | ||
| V7 | 1645486289896542336 | 0.697 | ab | 0.69019 | ab | ||
| V9* | 1645485430903072896 | 0.455 | c | – | – | 0.4555600 | d?** |
| V13 | 1645462001856973312 | 0.652 | ab | 0.64615 | ab | ||
| V16 | 1645469625423395712 | 0.291 | c | 0.68903 | ab | ||
| V21 | 1645461349021933696 | 0.679 | ab | 0.67487 | ab | ||
| V27 | 1645460760610869376 | 0.395 | c | 0.66343 | ab | ||
| V29 | 1645448356750244096 | 0.292 | c | 0.40963 | c | ||
| V47* | 1645446849212324992 | 0.615219 | ab | – | – | 0.6152161 | ab |
| V61 | 1645452067596906368 | 0.442 | c | 0.30569 | c | ||
| V67 | 1645437739590764416 | 0.714 | ab | 0.70698 | ab | ||
| V71*** | 1645451071164429824 | 0.659 | ab | 0.65512 | ab | ||
| V72 | 1645434887727621248 | 0.2035 | c | 0.59755 | ab | 0.59746 | ab |
| V76 | 1645354657738523008 | – | – | 0.63718 | ab | ||
| V79 | 1645461142863500928 | 0.458 | c | 0.31306 | c | ||
| V82 | 1645442171992256640 | 0.547 | ab | 0.54217 | ab | ||
| V92 | 1645360361455119744 | 0.518 | ab | 0.34110 | c | ||
| V93 | 1645340913846863232 | 0.676 | ab | 0.68137 | ab | ||
| V97 | 1645441038120910592 | 0.430093 | c | 0.75627 | ab | ||
| V98 | 1645440213487130624 | 0.259527 | c | 0.35055 | c |
Notes. (*)V9 and V47 are classified as ‘RR’ in the vari_classifier_result table only. Pulsation periods and other characteristics (amplitudes, mean magnitude, etc.) for these stars are from our analysis of their Gaia DR3 time series data.
(**)According to the long first–overtone period and the rather noisy light curve, V9 could be a double mode RR Lyrae star.
(***)The split light curve near the maximum light of V71 makes us suspect that it is a Blazhko RR Lyrae.
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