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Table 12.

Number of Cepheids within 2 kpc of the Sun.

Sample Method Fundamental mode Overtone Multi mode Total
Field LL WG
Field distance_gspphot
Field Parallax
Clusters LL WG, OGLE classifiers
Clusters LL WG, Gaia classifiers

Notes. The upper and lower indexes are an estimate of the maximum and minimum number of Cepheids, they are not standard errors, and for this reason, they are not are not added in quadrature.

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