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The Microfiche of Standard Stars

  • A. G. Davis Philip (a1)

Extract

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.

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References

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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.
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.

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