Implementaci\'on de un nuevo algoritmo de identificaci\'on de fuentes estelares en el c\'odigo SACAMAN
Abstract
An improved version of the identification stellar sources module in the quasi-automatic SACAMAN code is presented, which allows to obtain YZJHKs-VVV magnitudes for a set of predefined objects. The procedure uses a proximity algorithm 70 less time-consuming than the previous method of successive and counting approximation. This code is being applied to the study of variability of carbon stars belonging to the Galactic Bulge.
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