Datatype: PROC
The datatype proc refers to the membership probabilities
deduced from the location in the color magnitude diagram
(Photometric Probability) as published by
Kharchenko N., et al.
2005, Astron. Astrophys. 438, 1163
(2005A&A...438.1163K) and
2005, A&A 440, 403
(2005A&A...440..403K).
The Photometric probability Pph is calculated on the basis
of relative deviation of the colour-index (B-V) from the locus of cluster
members, including Pre-Main Sequence, Main Sequence stars and Red Giants
in the color-magnitude diagram for a given isochrone:
Pph = exp {-0.5 * [ d(B-V) / s(B-V) ] ^ 2 },
where s(B-V) is the the observational (B-V) error.
There is only one entry per star.
Record structure
| No | : | Star number |
|---|
| Ref | : | Data source |
|---|
| Prob | : | Membership probability |
|---|
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Last Update: 14 November 2005