MEGARA: the future IFU and MOS of the 10.4 M GTC


Autoria(s): 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
Data(s)

2013

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

http://eprints.ucm.es/38077/1/pascualramirez04libre.pdf

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