Abstract

The accuracy of locating weak photographic star images is described from a theoretical viewpoint. The objective is to determine the accuracy limitations imposed by the granular nature of the photographic image, by background radiation, and by image size and shape. After selecting models for both saturated and unsaturated images, lower bounds are derived for the rms location errors. These relationships are based on results developed for photoelectric images. The bounds apply to every method of interrogating the photographic images, and thus represent intrinsic limitations. For unsaturated images, the bound is a monotone function of the image “spread” σ; it is approximately proportional to σ(<i>c</i>-lnσ)<sup>-½</sup> where <i>c</i> is a constant. For saturated images, the bound is not necessarily a monotone function of the image spread. The bound may <i>decrease</i> as the image spread <i>increases</i>. The error bounds are compared to experimental errors. For an eighteenth-magnitude star, the bound is 70% of the experimental errors observed with plates from the 48-in. Schmidt telescope on Palomar.

PDF Article

References

  • View by:
  • |
  • |

  1. W. A. Baum, [Chapter 1] in Astronomical Techniques, edited by W. A. Hiltner (University of Chicago Press, Chicago, Illinois, 1962); J. C. Marchant and A. G. Millikan, J. Opt. Soc. Am. 55, 907 (1965); R. C. Jones, J. Opt. Soc. Am. 51, 1159 (1961).
  2. The effect of scanning a gaussian-shaped image with a rectangular aperture is described by E. J. Farrell and C. D. Zimmerman, in Optical and Electro-Optical Information Processing, edited by J. T. Tippett el al. (MIT Press, Cambridge, Massachusetts, 1965).
  3. W. A. Baum, Trans. Int. Astr. Un. 9, 681 (1955).
  4. E. J. Farrell, J. Opt. Soc. Am. 56, 578 (1966).
  5. Derivation given in reference cited in Ref. 4.
  6. See reference cited in Ref. 1.
  7. N. M. Evensen and R. E. Mohr investigated the characteristics of star images as a complement to a proper-motion survey being conducted by Professor Willem Luyten at the University of Minnesota.
  8. This relationship is developed by B. E. Bayer, J. Opt. Soc. Am. 54, 1485 (1964).
  9. For small values of r, I0(r)≍r/8.

Baum, W. A.

W. A. Baum, [Chapter 1] in Astronomical Techniques, edited by W. A. Hiltner (University of Chicago Press, Chicago, Illinois, 1962); J. C. Marchant and A. G. Millikan, J. Opt. Soc. Am. 55, 907 (1965); R. C. Jones, J. Opt. Soc. Am. 51, 1159 (1961).

W. A. Baum, Trans. Int. Astr. Un. 9, 681 (1955).

Bayer, B. E.

This relationship is developed by B. E. Bayer, J. Opt. Soc. Am. 54, 1485 (1964).

Evensen, N. M.

N. M. Evensen and R. E. Mohr investigated the characteristics of star images as a complement to a proper-motion survey being conducted by Professor Willem Luyten at the University of Minnesota.

Farrell, E. J.

E. J. Farrell, J. Opt. Soc. Am. 56, 578 (1966).

The effect of scanning a gaussian-shaped image with a rectangular aperture is described by E. J. Farrell and C. D. Zimmerman, in Optical and Electro-Optical Information Processing, edited by J. T. Tippett el al. (MIT Press, Cambridge, Massachusetts, 1965).

Mohr, R. E.

N. M. Evensen and R. E. Mohr investigated the characteristics of star images as a complement to a proper-motion survey being conducted by Professor Willem Luyten at the University of Minnesota.

Zimmerman, C. D.

The effect of scanning a gaussian-shaped image with a rectangular aperture is described by E. J. Farrell and C. D. Zimmerman, in Optical and Electro-Optical Information Processing, edited by J. T. Tippett el al. (MIT Press, Cambridge, Massachusetts, 1965).

Other (9)

W. A. Baum, [Chapter 1] in Astronomical Techniques, edited by W. A. Hiltner (University of Chicago Press, Chicago, Illinois, 1962); J. C. Marchant and A. G. Millikan, J. Opt. Soc. Am. 55, 907 (1965); R. C. Jones, J. Opt. Soc. Am. 51, 1159 (1961).

The effect of scanning a gaussian-shaped image with a rectangular aperture is described by E. J. Farrell and C. D. Zimmerman, in Optical and Electro-Optical Information Processing, edited by J. T. Tippett el al. (MIT Press, Cambridge, Massachusetts, 1965).

W. A. Baum, Trans. Int. Astr. Un. 9, 681 (1955).

E. J. Farrell, J. Opt. Soc. Am. 56, 578 (1966).

Derivation given in reference cited in Ref. 4.

See reference cited in Ref. 1.

N. M. Evensen and R. E. Mohr investigated the characteristics of star images as a complement to a proper-motion survey being conducted by Professor Willem Luyten at the University of Minnesota.

This relationship is developed by B. E. Bayer, J. Opt. Soc. Am. 54, 1485 (1964).

For small values of r, I0(r)≍r/8.

Cited By

OSA participates in CrossRef's Cited-By Linking service. Citing articles from OSA journals and other participating publishers are listed here.

Alert me when this article is cited.