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Título:
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MEGARA: the future IFU and MOS of the 10.4 M GTC
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Autores:
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Gil de Paz, Armando ;
Gallego Maestro, Jesús ;
Castillo Morales, África ;
Eliche Moral, María del Carmen ;
Marino, Raffaella Anna ;
Pascual Ramírez, Sergio ;
Zamorano Calvo, Jaime ;
Cardiel López, Nicolás ;
Pérez González, Pablo Guillermo ;
..., otros
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Tipo de documento:
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texto impreso
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Editorial:
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Universidad Nacional Autónoma Mexico, Inst. de Astronomía, 2013
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Dimensiones:
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application/pdf
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Nota general:
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info:eu-repo/semantics/openAccess
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Idiomas:
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Palabras clave:
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Estado = Publicado
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Materia = Ciencias: Física: Astrofísica
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Materia = Ciencias: Física: Astronomía
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Tipo = Artículo
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Resumen:
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In these proceedings we summarize the characteristics and current status of MEGARA, the future optical IFU and MOS for the 10.4 m GTC. MEGARA is being built by a Consortium led by the UCM (Spain) that also includes the INAOE (Mexico), the IAA-CSIC (Spain) and the UPM (Spain). The MEGARA IFU offers two different bundles, one called LCB with a field-of-view of 14 x 12 arcsec^2 and a spaxel size of 0.685 arcsec yielding spectral resolutions between R=6000-19000 and another one called SCB covering 10 x 8 arcsec^2 with 0.48 arcsec spaxels and resolutions R=8000-25000. The MOS component allows observing up to 100 targets in 3.5x3.5 arcmin^2. In September 2010 MEGARA was selected as the next optical spectrograph for GTC. Its PDR is scheduled for March 2012 with First Light on 2015.
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En línea:
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https://eprints.ucm.es/38077/1/pascualramirez04libre.pdf
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