Hostname: page-component-745bb68f8f-b95js Total loading time: 0 Render date: 2025-01-07T16:30:12.985Z Has data issue: false hasContentIssue false
  • English
  • Français

The Microfiche of Standard Stars

Published online by Cambridge University Press:  30 March 2016

A. G. Davis Philip
A. G. Davis Philip*
Affiliation:
Van Vleck Observatory and Union College

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

At the meeting, Calibration of Fundamental Stellar Quantities, IAU Symposium No. III held in Como, Italy in May, 1984, Philip and Egret (1985) suggested that the facilities of the Strasbourg Data Center be used to construct a microfiche of standard stars and other stars for which fundamental data have been obtained. A start had been made on this idea in Egret and Philip (1979) who published a microfiche, “Photometric Systems and Standard Stars” as part of the proceedings of the workshop “Problems of Calibration of Multicolor Photometric Photometry”. Now the plan is to expand this idea to cover standard stars in many systems and other stars for which fundamental data have been obtained.

Type
Joint Commission Meetings
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 847 - 852
Copyright
Copyright © Reidel 1986

References

Egret, D. and Philip, A. G. D. 1979 in Problems of Calibration of Multicolor Photometric Systems. Philip, A. G. D., ed., Dudley Obs. Rept. No. 14, microfiche.Google Scholar
Philip, A. G. D. and Egret, D. 1985 in IAU Symposium No. 111. Calibration of Fundamental Stellar Quantities. Hayes, D. S., Pasinetti, L. E. and Philip, A. G. D., eds., Reidel, Dordrecht, p. 353 and microfiche.Google Scholar