MEGARA Optics: Sub-aperture Stitching Interferometry for Large Surfaces

• Published in: Publications of the Astronomical Society of the Pacific 2018-04, Vol.130 (986), p.45001
• Main Authors: Aguirre-Aguirre, Daniel, Carrasco, Esperanza, Izazaga-Pérez, Rafael, Páez, Gonzalo, Granados-Agustín, Fermín, Percino-Zacarías, Elizabeth, de Paz, Armando Gil, Gallego, Jesús, Iglesias-Páramo, Jorge, Villalobos-Mendoza, Brenda
• Format: Article
• Language: English
• Subjects: Aperture; Astronomical instruments; instrumentation: miscellaneous; instrumentation: spectrographs; Interferometry; Optics; Spectroscopy; techniques: image processing
• ISSN: 0004-6280; 1538-3873
• DOI: 10.1088/1538-3873/aaa6b1

In this work, we present a detailed analysis of sub-aperture interferogram stitching software to test circular and elliptical clear apertures with diameters and long axes up to 272 and 180 mm, respectively, from the Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía (MEGARA). MEGARA is a new spectrograph for the Gran Telescopio Canarias (GTC). It offers a resolution between 6000 and 20000 via the use of volume phase holographic gratings. It has an integral field unit and a set of robots for multi-object spectroscopy at the telescope focal plane. The output end of the fibers forms the spectrograph pseudo-slit. The fixed geometry of the collimator and camera configuration requires prisms in addition to the flat windows of the volume phase holographic gratings. There are 73 optical elements of large aperture and high precision manufactured in Mexico at the Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE) and the Centro de Investigaciones en Óptica (CIO). The principle of stitching interferometry is to divide the surface being tested into overlapping small sections, which allows an easier analysis (Kim & Wyant 1981). This capability is ideal for non-contact tests for unique and large optics as required by astronomical instruments. We show that the results obtained with our sub-aperture stitching algorithm were consistent with other methods that analyze the entire aperture. We used this method to analyze the 24 MEGARA prisms that could not be tested otherwise. The instrument has been successfully commissioned at GTC in all the spectral configurations. The fulfillment of the irregularity specifications was one of the necessary conditions to comply with the spectral requirements.