EDP Sciences
Free access
Issue
A&A
Volume 390, Number 2, August I 2002
Page(s) 801 - 807
Section Instruments, observational techniques and data processing
DOI http://dx.doi.org/10.1051/0004-6361:20020740
Abstract : Optimum imaging observation wavelength

References

     
  • Fried, D. L. 1982, J. Opt. Soc. Am. 72, 52-61  
  • Greenwood, D. P. 1976, J. Opt. Soc. Am. 66, 193-206  
  • Hardy, J. W. 1998, Adaptive Optics for Astronomical Telescopes (New York, Oxford University Press)  
  • Jiang, W., Li, M., Tang, G., et al. 1995, Opt. Eng., 34, 15-20 NASA ADS  
  • Jiang, W., Ling, N., Tang, G., et al. 1998, SPIE Proc., 3353, 696-703  
  • Li, X., Jiang, W., Wang, C., & Xian, H. 2000, Acta Optica Sinica, 20, 10, 1328-1334  
  • Parenti, R. R., & Sasiela, R. J. 1994, J. Opt. Soc. Am. A, 11, 288-309  
  • Rao, C., Shen, F., & Jiang, W. 2000, Acta Optica Sinica, 20, 68-73  
  • Rimmele, T. R., & Radick, R. R. 1998, SPIE Proceedings, 3353, 72-81  
  • Roddier, F. 1981, The effects of atmospheric turbulence in optical astronomy, in Progress in Optics, ed. E. Wolf (North-Holland, Amsterdam), 19, 281-376  
  • Tyler, D. W., & Fender, J. S. 1994, SPIE Proceedings, 2201, 227-238  
  • Tyler, G. A. 1994, J. Opt. Soc. Am. A 11, 325-338  
  • Tyler, G. A. 1994, J. Opt. Soc. Am. A 11, 358-367

Abstract : Optimum imaging observation wavelength

Copyright ESO 2002