Table 2
The RR Lyr variable stars we have identified.
ID | αJ2000.0 | δJ2000.0 | Period | Type | ⟨ mF606W ⟩ | A F 606 W | ⟨ mF814W ⟩ | AF 814 W | ⟨ mV0 ⟩ | ⟨ mI0 ⟩ |
|
||||||||||
V1 | 0:42:46.9697 | 40:52:19.159 | 0.479 | RRab | 24.779 | 0.579 | 23.762 | – | – | – |
V2 | 0:42:47.2873 | 40:52:10.736 | 0.688 | RRab | 24.707 | 1.113 | 23.712 | – | – | – |
V3 | 0:42:47.0945 | 40:52:27.376 | 0.690 | RRab | 25.182 | 1.073 | 24.151 | – | – | – |
V4 | 0:42:47.9337 | 40:52:08.733 | 0.464 | RRab | 24.878 | 0.965 | 25.154 | – | – | – |
V5 | 0:42:48.0864 | 40:51:53.262 | 0.673 | RRab | 24.674 | 0.920 | 23.701 | – | – | – |
V6 | 0:42:46.1114 | 40:51:02.073 | 0.722 | RRab | 24.282 | 0.433 | 23.234 | – | – | – |
V7 | 0:42:48.1721 | 40:51:57.548 | 0.510 | RRab | 24.836 | 0.774 | 23.990 | – | – | – |
Notes. The mean F606W and F814W magnitudes are intensity-weighted over the light curve. V0 and I0 are the de-reddened mean magnitudes in the Johnson-Cousin photometric system obtained following the prescriptions by Sirianni et al. (2005). Type classification, RRab and RRc, indicate fundamental and first-overtone pulsation modes, respectively. The full table is available at the CDS.
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