Título

Segmented vortex telescope and its tolerance to diffraction effects and primary aberrations

Autor

JUAN PABLO TREVIÑO GUTIERREZ

Omar López Cruz

SABINO CHAVEZ CERDA

Nivel de Acceso

Acceso Abierto

Resumen o descripción

The segmented large millimeter telescope (LMT/GTM) is the largest spatial light modulator capable of producing vortex beams of integer topological charge. This observing mode could be applied for direct exoplanet searches in the millimeter or submillimeter regimes. The stability of the vortex structure against aberrations and diffraction effects inherent to the size and segmented nature of the collector mirror was studied. In the presence of low-order aberrations, the focal distribution of the system remains stable. Results show that these effects depend on the topological charge of the vortex and the relative orientation of the aberration with respect to the antenna axis. Coma and defocus show no large effects in the image at the focal plane; however, the system is very sensitive to astigmatism. Heat turbulence, simulated by random aberrations, shows that the system behaves in a similar way as astigmatism dissociating the vortices. The segmented vortex telescope is proposed as a novel approach for the detection of giant planets outside circumstellar disks around nearby stars. Since results are applicable to other facilities with segmented surfaces, it is suggested that this idea should be considered as a regular observation mode complementary to interferometric methods.

Editor

Optical Engineering

Fecha de publicación

21 de febrero de 2013

Tipo de publicación

Artículo

Versión de la publicación

Versión aceptada

Formato

application/pdf

Idioma

Inglés

Audiencia

Estudiantes

Investigadores

Público en general

Sugerencia de citación

Treviño, Juan P., et al., (2013), Segmented vortex telescope and its tolerance to diffraction effects and primary aberrations, Optical Engineering, Vol. 52(8):1-10

Repositorio Orígen

Repositorio Institucional del INAOE

Descargas

1067

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