MEGARA: the future IFU and MOS of the 10.4 M GTC
Data(s) |
2013
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Resumo |
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. |
Formato |
application/pdf |
Identificador | |
Idioma(s) |
en |
Publicador |
Universidad Nacional Autónoma Mexico, Inst. de Astronomía |
Relação |
http://eprints.ucm.es/38077/ http://www.astroscu.unam.mx/rmaa/RMxAC..42/PDF/RMxAC..42_agildepaz.pdf C DS00070-2006 S-2009/ESP-1496 |
Direitos |
info:eu-repo/semantics/openAccess |
Palavras-Chave | #Astrofísica #Astronomía |
Tipo |
info:eu-repo/semantics/article PeerReviewed |