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Commission 9: Instruments and Techniques (Instruments et Techniques)

Published online by Cambridge University Press:  25 April 2016

John Davis

Extract

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The period covered by this report has seen significant progress in the development of the new generation of telescopes with apertures in the 8 m plus range. The period has encompassed the major construction phase of the 10 m Keck Telescope, witnessed the commissioning of the European Southern Observatory’s (ESO) New Technology Telescope and the approval of funding for the ESO Very Large Telescope (VLT). Significant progress has been achieved in developing the necessary technology for manufacturing and figuring large mirrors. There have been major expansions of activity in the areas of active control of telescope optics and adaptive optics, and in high angular resolution interferometry with several new groups entering both fields. The use of optical fibers, particularly in the area of multiple-object spectroscopy, has continued to grow. Several telescopes can now be operated remotely and the control systems of new telescopes are being designed to facilitate remote operation.

Type
Research Article
Information
Transactions of the International Astronomical Union , Volume 21 , Issue 1 , 1991 , pp. 41 - 52
Copyright
Copyright © Kluwer 1991

References

Babcock, H.W., 1990. “Adaptive Optics Revisited”. Science, 249, 253–257.Google Scholar
Bagnuolo, W.G., Furenlid, I.K., Gies, D.R., Barry, D.J., Russell, W.H., Dorsey, J.F., 1990. “The Multi-Telescope Telescope: A Cost-Effective Approach to Fiber-Fed Spectroscopy”. Publ. Astron. Soc. Pacific, 102, 604–611.Google Scholar
Buscher, D.F., Haniff, C.A., Baldwin, J.E., Warner, P.J., 1990. “Detection of a bright feature on the surface of Betelgeuse”. Mon. Not. R. Astron. Soc., 245, 7P–11P.Google Scholar
Forbes, F., Roddier, F., Poczulp, G., Sweeny, G., Dueck, R., 1989. “Segmented bimorph deformable mirror”. J. Phys. E: Sci. Instrum., 22, 402–405.Google Scholar
Lacy, J.H., Achtermann, J.M., Bruce, D.E., Lester, D.F., Arens, J.F., Peck, M.C., Gaalema, S.D., 1989. “IRSHELL: A Mid-Infrared Cryogenic Echelle Spectrograph”. Publ. Astron. Soc. Pacific, 101, 1166–1175.Google Scholar
Nather, R.E., Winget, D.E., Clemens, J.C., Hansen, C.J., Hine, B.P., 1990. “The Whole Earth telescope: A New Astronomical Instrument”. Astrophys. J., (in press).CrossRefGoogle Scholar
Papaliolios, C., Nisenson, P., Ebstein, S., 1985. “Speckle imaging with the PAPA detector”. Applied Optics, 24, 287–292.Google Scholar
Rousset, G., Fontanella, J.C., Kern, P., Gigan, P., Rigaut, , Lena, P., Boyer, C., Jagourel, P., Gaffard, J.P., & Merkle, F., 1990. “First diffraction-limited astronomical images with adaptive optics”. Astron. Astrophys., 230, L29–32.Google Scholar
Roddier, F., 1988. “Curvature sensing and compensation: a new concept in adaptive optics”. Applied Optics, 27, 1223–1225.Google Scholar