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Fig. 27.
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Distribution in G magnitude of the clean sample of 270 905 DR3 RR Lyrae stars confirmed with the SOS Cep&RRL pipeline. The peaks at G∼ 19.2, 19.7 mag correspond to RR Lyrae stars in the LMC and SMC, respectively. The magnitude distribution of the 70 611 new RR Lyrae stars is highlighted in black.
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