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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.

(a)

For one-filter RR Lyr we have only one mean magnitude, thus we can not estimate the corresponding amplitude or Johnson-Cousin magnitudes, we can only indicate the Dolphot mean magnitude.

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