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Making observations with GTC/MEGARA easier: the MEGARA observing preparation software suite

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Eliche Moral, María del Carmen and Pascual Ramírez, Sergio and Gruel, N. and Castillo Morales, África and Carrasco, E. and Gallego Maestro, Jesús and García Vargas, M. L. and Gil de Paz, Armando and Marino, Raffaella Anna and Morales, I. and Pérez Calpena, A. and Sánchez, F. M. and Vílchez, J. M. and Villar, V. and Zamorano Calvo, Jaime (2013) Making observations with GTC/MEGARA easier: the MEGARA observing preparation software suite. Revista Mexicana de astronomía y astrofísica, 42 . p. 125. ISSN 0185-1101

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Official URL: http://www.astroscu.unam.mx/rmaa/RMxAC..42/PDF/RMxAC..42_meliche2.pdf


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Abstract

MEGARA (Multi-Espectrografo en GTC de Alta Resolucion para Astronomia) is an optical Integral-Field Unit (IFU) and Multi-Object Spectrograph (MOS) designed for the GTC 10.4 m telescope in La Palma. Its relatively complex layout makes necessary a set of tools to facilitate the observation preparation to the user. The MEGARA Observing Preparation Software Suite (MOPSS) consists on three software components designed to assist observers to optimally plan their observations with GTC/MEGARA: the Exposure Time Calculator, the Image Simulator, and the Fiber MOS Positioning tool. We describe these software tools and the status of their prototypes up to the date.


Item Type:Article
Additional Information:

© 2013: Instituto de Astronomía, UNAM.
Science with the GTC Meeting (4th. 2011. Santa Cruz La Palma, Spain).
Supported by the Spanish Ministry of Science and Innovation (MICINN) under projects AYA2009- 10368, AYA2006-12955, and AYA2009-11137, and by the Madrid Regional Government through the AstroMadrid Project (CAM S2009/ESP-1496). Funded by the Spanish MICINN under the ConsoliderIngenio 2010 Program grant CSD2006-00070: “First Science with the GTC”. S. D. H. & G.

Uncontrolled Keywords:Astronomy & Astrophysics
Subjects:Sciences > Physics > Astrophysics
Sciences > Physics > Astronomy
ID Code:38124
Deposited On:16 Jun 2016 15:32
Last Modified:10 Dec 2018 15:05

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