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Table 1

List of candidate cluster positions, apparent radii, AKs, and modulus distances (DM).

ID RA(J2000)a Dec(J2000)a radius AKs field b DM(⟨ AKs field ⟩ )c AKs cRSGs d DM(AKs RSGs)e DM(red clump)f DM(Sp)g
[ hh mm ss ] [°′′] [′′] [ mag ] [ mag ] [ mag ] [ mag ] [ mag ] [ mag ]

cl1.5 17 53 45.09 –28 11 08.29 73 0.45 ± 0.08 (12.7 ± 0.2) ··· ··· 14.54 ± 0.16 ···
cl9.5 18 10 54.34 –21 12 37.67 60 0.70 ± 0.11 (13.3 ± 0.2) ··· ··· 14.05 ± 0.12 ···
cl16.7 18 23 34.40 –14 39 10.86 76 0.44 ± 0.27 12.7 ± 0.9 0.49 ± 0.03 12.8 ± 0.1 12.93 ± 0.13 ···
cl49.3 19 19 31.53 14 54 08.57 130 0.48 ± 0.35 13.8 ± 1.9 0.47 ± 0.11 13.7 ± 0.5 14.22 ± 0.12 14.16 ± 1.00
cl59.8 19 46 18.57 23 22 30.23 85 0.26 ± 0.17 12.9 ± 1.4 ··· ··· ··· ···

Notes.

(a)

Positions are derived as the centroid of surface brightness maps from 2MASS Ks band images.

(b)

AKs field is the average AKs of the spectroscopically observed late-type stars in the field.

(c)

DM(AKs field) is the distance modulus obtained from the AKs values of detected late-type stars and the model of Drimmel et al. (2003).

(d)

AKs RSGs is the average AKs of the detected RSGs.

(e)

DM(AKs RSGs) is the distance modulus obtained from the AKs values of cRSGs and the model of Drimmel et al. (2003).

(f)

DM(red clump) is the distance modulus obtained from the AKs values of cRSGs and field red clump stars.

(g)

DM(Sp): spectro-photometric distance modulus of star 39, by assuming a giant case (O9.5-B3III). For a dwarf case, DM would be 13.02 ± 0.77 mag.

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