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MEGARA: the future optical IFU and multi-object spectrograph for the 10.4m GTC Telescope

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Gil de Paz, Armando and Gallego Maestro, Jesús and Castillo Morales, África and Eliche Moral, María del Carmen and Pascual, S. and Sánchez Penim, A. and Villar, V. and Zamorano Calvo, Jaime and Cardiel López, Nicolás and Cava, A. and Pérez González, Pablo Guillermo (2012) MEGARA: the future optical IFU and multi-object spectrograph for the 10.4m GTC Telescope. Proceedings of SPIE, 8446 . ISSN 0277-786X

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Official URL: http://dx.doi.org/10.1117/12.925739




Abstract

In these proceedings we give a summary of the characteristics and current status of the MEGARA instrument, the future optical IFU and MOS for the 10.4-m Gran Telescopio Canarias (GTC). MEGARA is being built by a Consortium of public research institutions led by the Universidad Complutense de Madrid (UCM, Spain) that also includes INAOE (Mexico), IAA-CSIC (Spain) and UPM (Spain). The MEGARA IFU includes two different fiber bundles, one called LCB (Large Compact Bundle) with a field-of-view of 12.5x11.3 arcsec(2) and a spaxel size of 0.62 arcsec yielding spectral resolutions between R=6,800-17,000 and another one called SCB (Small Compact Bundle) covering 8.5x6.7 arcsec(2) with hexagonally-shaped and packed 0.42-arcsec spaxels and resolutions R=8,000-20,000. The MOS component allows observing up to 100 targets in 3.5x3.5 arcmin(2). Both the IFU bundles and the set of 100 robotic positioners of the MOS will be placed at one of the GTC Folded-Cass foci while the spectrographs (one in the case of the MEGARA-Basic concept) will be placed at the Nasmyth platform. On March 2012 MEGARA passed the Preliminary Design Review and its first light is expected to take place at the end of 2015.


Item Type:Article
Additional Information:

© 2012 SPIE. Conference on Ground-Based and Airborne Telescopes (4º. 2012. Amsterdam, Netherlands). This project is partly funded by the Spanish Ministry of Science and Innovation (MICINN) under project AYA2009-10368, by the Madrid Regional Government through the AstroMadrid Project (CAM S2009/ESP- 1496) and by the Spanish MICINN under the Consolider Ingenio 2010 Program grant CSD2006-00070: First Science with the GTC. This work is being done in the framework of the Moncloa Campus of International Excellence (UCM-UPM).

Uncontrolled Keywords:Galaxy formation; Spiral galaxies; Disk; Evolution; Profiles; Regions
Subjects:Sciences > Physics > Astrophysics
Sciences > Physics > Astronomy
Sciences > Physics > Atmospheric physics
ID Code:27828
Deposited On:13 Jan 2015 08:41
Last Modified:10 Dec 2018 15:05

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