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The identification of the variable stars published on IBVS #3573 has ben revised on the basis of the original (unpublished) finding charts.Cross check with the 2MASS catalog has been made to get more accurate coordinates and to confirm their nature from their J -H, H -K colors.The Mira stars, given their known periods, could be used with the astrometric parallaxes of the forthcoming Gaia catalog to improve the Period-Luminosity relation.
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R. Nesci (2018) studied this question.
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