Table A.1
23 PNe observed in the sample.
| Source name | Source PNG | RA (J2000) | Dec (J2000) | AORkey | AORKey | Rg |
|---|---|---|---|---|---|---|
| (h m s) | (d m s) | off position | (kpc) | |||
| J320 | 190.3 − 17.7 | 05 05 34.32 | + 10 42 23.8 | 21 946 880 | 21 947 136 | 13.6 ± 1.6 |
| K3-65 | 153.7 − 01.4 | 04 15 54.53 | + 48 49 40.1 | 21 947 392 | 21 947 648 | 11.5 ± 2.1* |
| K3-66 | 167.4 − 09.1 | 04 36 37.23 | + 33 39 30.0 | 21 947 904 | 21 948 160 | 15.8 ± 2.3 |
| K3-67 | 165.5 − 06.5 | 04 39 47.93 | + 36 45 42.6 | 21 948 416 | 21 948 672 | 14.4 ± 4.3† |
| K3-68 | 178.3 − 02.5 | 05 31 35.86 | + 28 58 41.6 | 21 948 928 | 21 949 184 | 10.2 ± 1.8* |
| K3-69 | 170.7 + 04.6 | 05 41 22.13 | + 39 15 08.1 | 21 949 440 | 21 949 696 | >13.9* |
| K3-70 | 184.6 + 00.6 | 05 58 45.34 | + 25 18 43.8 | 21 949 952 | 21 950 208 | >14.0* |
| K3-71 | 184.8 + 04.4 | 06 13 54.98 | + 26 52 57.0 | 21 950 464 | 21 950 720 | 10.5 ± 2.0* |
| K3-90 | 126.3 + 02.9 | 01 24 58.70 | + 65 38 34.7 | 21 950 976 | 21 951 232 | <8.7* |
| K4-48 | 201.7 + 02.5 | 06 39 55.84 | + 11 06 30.3 | 21 952 000 | 21 952 256 | 16.6 ± 5.0† |
| M1-1 | 130.3 − 11.7 | 01 37 19.43 | + 50 28 11.6 | 21 952 512 | 21 952 768 | 14.7 ± 2.4 |
| M1-6 | 211.2 − 03.5 | 06 35 45.13 | − 00 05 37.5 | 21 953 024 | 21 953 280 | 9.8 ± 1.8* |
| M1-7 | 189.8 + 07.7 | 06 37 20.96 | + 24 00 35.4 | 21 953 536 | 21 953 792 | 14.5 ± 1.9 |
| M1-8 | 210.3 + 01.9 | 06 53 33.79 | + 03 08 27.0 | 21 954 048 | 21 954 304 | 12.2 ± 1.4 |
| M1-9 | 212.0 + 04.3 | 07 05 19.20 | + 02 46 59.5 | 21 954 560 | 21 954 816 | 16.2 ± 2.5 |
| M1-14 | 234.9 − 01.4 | 07 27 56.50 | − 20 13 22.8 | 21 955 072 | 21 955 328 | 11.4 ± 1.1 |
| M1-16 | 226.7 + 05.6 | 07 37 18.93 | − 09 38 48.0 | 21 955 584 | 21 955 840 | 13.0 ± 1.8 |
| M1-17 | 228.8 + 05.3 | 07 40 22.19 | − 11 32 29.9 | 21 956 096 | 21 956 352 | 14.8 ± 2.3 |
| M2-2 | 147.8 + 04.1 | 04 13 15.04 | + 56 56 58.1 | 21 956 608 | 21 956 864 | >9.7* |
| M3-2 | 240.3 − 07.6 | 07 14 49.92 | − 27 50 23.3 | 21 957 120 | 21 957 376 | 15.3 ± 2.6 |
| M4-18 | 146.7 + 07.6 | 04 25 50.85 | + 60 07 12.8 | 21 957 632 | 21 957 888 | 15.0 ± 2.2 |
| SaSt2-3 | 232.0 + 05.7 | 07 48 03.67 | − 14 07 40.4 | 21 958 144 | 21 958 400 | 20.8 ± 4.1 |
| Y-C 2-5 | 240.3 + 07.0 | 08 10 41.64 | − 20 31 32.6 | 21 958 656 | 21 958 912 | 13.2 ± 6.6‡ |
Notes. Galactocentric distances and their errors were determined from heliocentric values determined statistically from Frew et al. (2016), assuming Rg,⊙ =8.0 ± 0.5 kpc, except: * directly measured distances from Giammanco et al. (2011); † statistical distances from Phillips & Márquez-Lugo (2011); ‡ statistical distance from Costa et al. (2004), from which we assume a 50% error.
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