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Table 3.

Mean differences between APASS and the Carrasco transformation polynomials and our own photometry.

Cluster APASS Gaia
ΔV ΔB Δ(B − V) N ΔV ΔB Δ(B − V) N
vdBH 73 −0.07 ± 0.05 −0.04 ± 0.05 0.03 ± 0.03 301 −0.03 ± 0.03 −0.01 ± 0.07 0.01 ± 0.07 95
vdBH 85 0.01 ± 0.04 0.03 ± 0.05 0.03 ± 0.04 32 0.01 ± 0.02 0.02 ± 0.07 0.00 ± 0.07 11
RUP 87 −0.02 ± 0.05 0.01 ± 0.09 0.02 ± 0.07 41 0.00 ± 0.02 0.00 ± 0.03 0.00 ± 0.04 17
RUP 85 −0.04 ± 0.05 −0.02 ± 0.10 0.02 ± 0.08 36 −0.01 ± 0.02 0.02 ± 0.03 0.03 ± 0.03 22
vdBH 87 −0.03 ± 0.05 −0.02 ± 0.06 0.01 ± 0.04 37 −0.02 ± 0.03 0.02 ± 0.06 0.04 ± 0.08 18
vdBH 92 −0.06 ± 0.05 −0.05 ± 0.06 0.01 ± 0.04 34 −0.02 ± 0.04 0.02 ± 0.07 0.03 ± 0.04 20
TR 12 −0.07 ± 0.07 −0.07 ± 0.07 0.00 ± 0.05 37 −0.01 ± 0.04 −0.03 ± 0.09 −0.02 ± 0.07 29
vdBH 91 −0.06 ± 0.06 −0.04 ± 0.09 0.02 ± 0.05 81 −0.01 ± 0.02 0.00 ± 0.04 0.01 ± 0.05 33
TR 13 −0.13 ± 0.10 −0.08 ± 0.07 0.05 ± 0.05 38 −0.04 ± 0.03 0.01 ± 0.10 0.04 ± 0.10 42
vdBH 106 −0.07 ± 0.08 −0.07 ± 0.08 −0.01 ± 0.06 44 −0.01 ± 0.01 −0.04 ± 0.04 −0.03 ± 0.04 12
RUP 88 −0.06 ± 0.05 −0.04 ± 0.07 0.02 ± 0.04 44 −0.01 ± 0.01 −0.02 ± 0.06 −0.01 ± 0.06 29
RUP 162 −0.16 ± 0.14 −0.13 ± 0.19 0.04 ± 0.10 20 −0.02 ± 0.05 0.02 ± 0.14 0.04 ± 0.11 28
Lynga15 −0.08 ± 0.08 −0.09 ± 0.06 −0.01 ± 0.07 98 −0.06 ± 0.04 −0.06 ± 0.09 0.00 ± 0.07 53
Loden 565 −0.03 ± 0.04 −0.02 ± 0.07 0.00 ± 0.04 43 −0.01 ± 0.03 0.01 ± 0.04 0.02 ± 0.04 23
NGC 4230 −0.03 ± 0.04 0.00 ± 0.06 0.03 ± 0.04 23 −0.03 ± 0.02 0.02 ± 0.10 0.05 ± 0.10 11
NGC 4349 −0.11 ± 0.08 −0.10 ± 0.09 0.01 ± 0.07 296 −0.05 ± 0.04 −0.03 ± 0.09 0.02 ± 0.08 131

Notes. The columns named N show the number of stars that were used to estimate these values for each cluster.

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