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This thesis project arises from the need to put into operation thespectrograph (COLORES) of the station (BOOTES 2), located in La Mayora andbelonging to the network of Burst Observer and Optical Transient ExploringSystem (BOOTES) telescopes. A robotic telescope such as the one located atBOOTES 2 has, among its many virtues, the ability to perform a multitude ofobservations with a very low reaction time. This makes it possible to obtain alarge amount of data on the positioning and characterization of astronomicalbodies. With this tool in operation, it will now be possible to extract amultitude of new parameters from the observations, providing this station witha more complete and versatile instrument with which to obtain more interestingscientific information.  For this task, a series of scripts will be performed. Specifically two, onefor the calibration of the spectrograph and another one in charge of the imageprocessing and the extraction of its spectrum. This will be carried out usingSpyder software (Python), in which, in addition, numerous tests will be carriedout to verify that the software works perfectly. Once these tests have beencarried out, it will be implemented in the telescope's Web page for its use.  Several libraries will be used for this purpose, including Astropy, whichincludes a complete package for handling astronomical data in Python, andMatplotlib, which allows the use of graphics generated from data contained inarrays. In addition, several image acquisition techniques will be used, suchas: filtering, Gaussian adjustment, and use of regions of interferences. Withall this, the data extracted from the telescope will be optimized to achievethe desired results.

Desarrollo del software de interfaz de usuario para el espectr\'ografo astron\'omico COLORES instalado en el observatorio de la Mayora