Hostname: page-component-68945f75b7-zpsnj Total loading time: 0 Render date: 2024-08-05T11:21:03.625Z Has data issue: false hasContentIssue false
  • English
  • Français

Objective and Consistent Stellar Magnitudes from the Palomar Sky Survey Prints

Published online by Cambridge University Press:  25 April 2016

G. L. White
G. L. White*
Affiliation:
School of Physics, University of Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

Print copies of the Palomar Sky Survey (PSS) are widely used for optical identifications of radio sources north of δ = -33°.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 88 - 90
Copyright
Copyright © Astronomical Society of Australia 1980

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Hawkins, M. R. S., Mon. Not. R. Astron. Soc., 188, 691 (1979).CrossRefGoogle Scholar
Hayman, P. G., Hazard, C., and Sanitt, N., Mon. Not. R. Astron. Soc., 189, 853 (1979).CrossRefGoogle Scholar
Hazard, C., and Murdoch, H. S., Aust. J. Phys. Astrophys. Suppl. 1, No. 42 (1977).Google Scholar
Minkowski, R. L., and Abell, G. O. in Basic Astronomical Data, p. 481, (ed. Strand, K. Aa., Chicago University Press) (1963).Google Scholar
Pěkný, Zd., Bull. Astron. Inst. Czech., 9, 164 (1958).Google Scholar
Perek, L., Bull. Astron. Inst. Czech., 9, 39 (1958).Google Scholar
Peterson, B. A., Bolton, J. G., and Shimmins, A. J., Astrophys. Lett., 15, 109 (1973).Google Scholar
Plaut, L., Bull. Astron. Inst. Neth., Suppl. 1, 105 (1966).Google Scholar
White, G. L., Mon Not. R. Astron. Soc. (1980) (in press).Google Scholar
White, G. L., Murdoch, H. S., and Hunstead, R. W., Mon. Not. R. Astron. Soc. (1980) (in press).Google Scholar