<transcript><audio_80> librería fotométrica y espectral de estrellas variables pero no cualquier tipo de estrellas variables, tienen que ser estrellas variables brillantes, ¿por qué brillantes? porque eso depende de los instrumentos de observación</transcript><transcript><audio_81> Ahorita contamos con un telescopio de apertura pequeña que es alrededor de 8 pulgadas, tiene una montura ecuatorial y tenemos una cámara CCD</transcript><transcript><audio_82> ahorita es monitorear este tipo de estrellas sin filtro. ¿Por qué sin filtro? Porque queremos intentar calibrar y sistematizar todo el proceso de reducción de imágenes. Hasta el momento,</transcript><transcript><audio_83> creo que ya contamos al menos con tres estrellas observadas y con periodos ya establecidos y una de ellas es roo poop is a roo poop is es una estrella tipo delta scuti delta scuti se encuentra en esta región del</transcript> is to create a photometric and spectral library of  variable stars but not just any type of variable stars they have to be bright variable stars because bright because that depends on the observation instruments that we have right now we have a small aperture telescope that is around 8 inches it has an equatorial mount and we have a right now what we want to do right now is monitor this type of stars without a filter because without a filter because we want to try to calibrate and systematize the entire image reduction process so far we already have at least I think we already have at least  three stars observed and with periods already established and one of them closed popis arropó peace is a type star of the test cut and the test cut and is located in this region
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