Bibcode
Garzón, F.; Abreu, D.; Barrera, S.; Becerril, S.; Cairós, L. M.; Díaz, J. J.; Fragoso, A. B.; Gago, F.; Grange, R.; González, C.; López, P.; Patrón, J.; Pérez, J.; Rasilla, J. L.; Redondo, P.; Restrepo, R.; Saavedra, P.; Sánchez, V.; Tenegi, F.; Vallbé, M.
Referencia bibliográfica
First Light Science with the GTC (Eds. R. Guzmán, C. Packham, J. M. Rodríguez-Espinosa, & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 29, pp. 12-17 (2007) (http://www.astroscu.unam.mx/~rmaa/)
Fecha de publicación:
6
2007
Número de citas
4
Número de citas referidas
2
Descripción
EMIR, currently entering into its fabrication and AIV phase, will be one
of the first common user instruments for the GTC, the 10 meter telescope
under construction by GRANTECAN at the Roque de los Muchachos
Observatory (Canary Islands, Spain). EMIR is being built by a Consortium
of Spanish and French institutes led by the Instituto de
Astrofísica de Canarias (IAC). EMIR is designed to realize one of
the central goals of 10m class telescopes, allowing observers to obtain
spectra for large numbers of faint sources in a time-efficient manner.
EMIR is primarily designed to be operated as a MOS in the K band, but
offers a wide range of observing modes, including imaging and
spectroscopy, both long slit and multi-object, in the wavelength range
0.9 to 2.5 μm. It is equipped with two innovative subsystems: a
robotic reconfigurable multi-slit mask and dispersive elements formed by
the combination of high quality diffraction grating and conventional
prisms, both at the heart of the instrument. The present status of
development, expected performances, schedule and plans for scientific
exploitation are described and discussed. The development and
fabrication of EMIR is funded by GRANTECAN and the Plan Nacional de
Astronomía y Astrofísica (National Plan for Astronomy and
Astrophysics, Spain).