Pascual Ramírez, SergioGallego Maestro, JesúsCardiel López, NicolásEliche Moral, María del Carmen2023-06-202023-06-2020130185-1101https://hdl.handle.net/20.500.14352/45080© 2013: Instituto de Astronomía, UNAM. Science with the GTC Meeting (4th. 2011. Santa Cruz La Palma, SPAIN).The UCM Instrumentation Group (GUAIX) is developing currently Data Reduction Pipelines (DRP) for four instruments of the GTC: EMIR, FRIDA, MEGARA and MIRADAS. The purpose of the DRPs is to provide astronomers scientific quality data, removing instrumental biases, calibrating the images in physical units and providing a estimation of the associated uncertainties.engjournal articlehttp://www.astroscu.unam.mx/rmaa/RMxAC..42/PDF/RMxAC..42_spascual.pdfopen access52Astronomy & AstrophysicsAstrofísicaAstronomía (Física)