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Table 2.
Limiting fluxes for all clusters, calculated using a broad emission line (40 Å) and also valid for narrow lines (see text).
Cluster | log10Fmin [erg s−1 cm−2 Å−1] |
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---|---|---|---|
MS | TO | RGB | |
NGC 104 | ![]() |
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NGC 1851 | ![]() |
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NGC 1904 | ![]() |
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NGC 2808 | ![]() |
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NGC 3201 | ![]() |
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NGC 362 | ![]() |
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NGC 5139 | ![]() |
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NGC 5286 | ![]() |
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NGC 5904 | ![]() |
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NGC 6093 | ![]() |
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NGC 6121 | ![]() |
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NGC 6218 | ![]() |
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NGC 6254 | ![]() |
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NGC 6266 | ![]() |
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NGC 6293 | ![]() |
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NGC 6388 | ![]() |
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NGC 6441 | ![]() |
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NGC 6522 | ![]() |
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NGC 6541 | ![]() |
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NGC 6624 | ![]() |
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NGC 6656 | ![]() |
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NGC 6681 | ![]() |
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NGC 6752 | ![]() |
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NGC 7078 | ![]() |
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NGC 7089 | ![]() |
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NGC 7099 | ![]() |
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Notes. Uncertainties give the central 80% of the distribution on the main-sequence (MS), main-sequence turn-off (TO), and red giant branch (RGB).
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