Implementación de un nuevo algoritmo de identificación de fuentes estelares en el código 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 $\simeq$ 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.

arXiv comment4 pages, in Spanish; Proceeding of 3rd Conference on Stellar Astrophysics, in honor of the trajectory of Professor Juan José Clariá, Córdoba (Argentina), June 21st-24th, 2016