University of Mexico adaptive optics program


Por: Cuevas S., Sotelo P.D., Garfias F., Iriarte Valverde A.I., Martinez L.A., Orlov V.G., VOYTSEKHOVICH, VALERY, Chapa O., Tinoco S.J., Vernin J., Avila R., Marchis F., Graves J.E., Northcott M.J., Roddier F.J., Roddier C.A.

Publicada: 1 ene 1998
Resumen:
We describe different works conducing to the adaptive optics system for the TIM 6.5m telescope. We show turbulence profiles result at our San Pedro Martir Observatory in Baja using the Generalized SCIDAR. We can conclude that the turbulence conditions in this site are comparable to the major observatories in the world. From these results and taken in account curvature AO simulations it is possible to predict the performances in limiting magnitude and sky coverage of different AO systems and telescopes in our observatory. We can also define the degree of the AO system for the TIM 6.5m telescope. We made a short description of our LOLA tip-tilt corrector system and the GUIELOA 19 elements curvature AO system. The calculation of the optics quality for the TIM 6.5m is briefly mentioned. Studies about the influence of the finite outerscale on the optical quality of AO corrected images are described. ©2003 Copyright SPIE - The International Society for Optical Engineering.

Filiaciones:
Cuevas S.:
 Instituto de Astronoinia UNAM, 04510 Ciudad Universitaria, Apdo. Postal 70-264, D.F., Mexico, Mexico

Sotelo P.D.:
 Instituto de Astronoinia UNAM, 04510 Ciudad Universitaria, Apdo. Postal 70-264, D.F., Mexico, Mexico

Garfias F.:
 Instituto de Astronoinia UNAM, 04510 Ciudad Universitaria, Apdo. Postal 70-264, D.F., Mexico, Mexico

Iriarte Valverde A.I.:
 Instituto de Astronoinia UNAM, 04510 Ciudad Universitaria, Apdo. Postal 70-264, D.F., Mexico, Mexico

Martinez L.A.:
 Instituto de Astronoinia UNAM, 04510 Ciudad Universitaria, Apdo. Postal 70-264, D.F., Mexico, Mexico

Orlov V.G.:
 Instituto de Astronoinia UNAM, 04510 Ciudad Universitaria, Apdo. Postal 70-264, D.F., Mexico, Mexico

Chapa O.:
 Instituto de Astronoinia UNAM, 04510 Ciudad Universitaria, Apdo. Postal 70-264, D.F., Mexico, Mexico

Vernin J.:
 Departement d'Astrophysique, Universite de Nice, U.R.A. 709 du CNRS, F-06108 Nice Cedex 2, France

Avila R.:
 Departement d'Astrophysique, Universite de Nice, U.R.A. 709 du CNRS, F-06108 Nice Cedex 2, France

Marchis F.:
 European Southern Observatory, Alonso de Cordova 310, Vitacura P.O. 19001 Santiago 19, Chile

Graves J.E.:
 Institut for Astronomy, University of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96825, United States

Northcott M.J.:
 Institut for Astronomy, University of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96825, United States

Roddier F.J.:
 Institut for Astronomy, University of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96825, United States

Roddier C.A.:
 Institut for Astronomy, University of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96825, United States
ISSN: 0277786X
Editorial
SPIE-INT SOC OPTICAL ENGINEERING, 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA, Estados Unidos America
Tipo de documento: Conference Paper
Volumen: 3353 Número:
Páginas: 531-542
WOS Id: 000076793400059

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