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Table A.2.

Astrometric parameters of the 405 PNe from the GAPN-EDR3 sample.

PNG Name Parallax ER paral. Distance Low dist. High dist. < z> < R> ang < R> phy Velrad Morph. Spec. type
(mas) (mas) (pc) (pc) (pc) (pc) (as) (pc) (km/s)
PN G000.3+12.2 0.414 0.053 2456 2224 2735 520 6.8 0.081 -34 B O(H)3 If
PN G000.3-04.2 0.207 0.047 5676 4518 7107 -418 18 0.495 R
PN G001.0+01.4 0.749 0.067 1342 1228 1468 35 16.1 0.105 E
PN G002.0-06.2 0.283 0.051 3852 3251 4559 -418 2.6 0.049 -119 E O5f(H)
PN G002.4+05.8 0.963 0.06 1053 1005 1116 107 14.8 0.075 -106 E [WO 3]
PN G002.4-03.4 0.256 0.033 4084 3624 4701 -247 7.8 0.153 E
PN G002.4-03.7 0.163 0.031 6067 5181 6819 -396 1.8 0.051 -92 S O(H)7-8
PN G002.7-52.4 0.862 0.056 1167 1104 1236 -925 65.1 0.368 -26 R hgO(H)
PN G002.9+06.5 0.238 0.048 4803 3896 5714 549 2.5 0.058 70 R
PN G003.3+66.1 1.482 0.242 729 603 905 667 23.8 0.084 -17 R DAO
PN G003.3-04.6 0.157 0.025 6586 5595 7376 -535 5.3 0.168 157 E B0I-III
PN G003.4+01.4 0.508 0.078 2131 1870 2477 52 7.5 0.077 E
PN G006.4-03.4 0.204 0.049 5473 4484 6638 -331 13.5 0.358 E
PN G006.9-30.2 2.916 0.048 342 337 346 -172 7650 12.691
PN G007.0+06.3 0.219 0.05 4761 4147 5761 525 3.2 0.074 -26 E
PN G007.9+10.1 0.269 0.047 3954 3432 4742 697 3.6 0.069 -45 S
PN G009.1-03.4 0.28 0.062 4099 3446 5172 -245 44.5 0.884 I
PN G009.4-05.5 0.523 0.024 1943 1873 2043 -171 8 0.076 13 E [WC5/6]
PN G009.6+14.8 0.408 0.078 2580 2195 3030 660 8.8 0.11 -40 B O(He)
PN G010.8-01.8 0.412 0.049 2484 2255 2728 -79 6 0.072 5 E Of
PN G011.3+02.8 0.293 0.053 3668 3103 4321 182 2.5 0.044 -62
PN G011.7-00.6 0.392 0.043 2568 2362 2798 -29 3.6 0.045 120 E [WC5/6]
PN G011.7-41.3 2.34 0.048 428 420 437 -283 600 1.245 sdO
PN G011.8+03.7 0.606 0.036 1662 1572 1750 110 19 0.153 E
PN G012.1-11.2 0.183 0.036 5605 4588 7160 -1091 9.6 0.262 E O(H)6III-V
PN G013.8-02.8 0.572 0.077 1913 1676 2214 -94 47.5 0.441 B
PN G014.0-02.5 0.277 0.07 3924 3181 4828 -173 3 0.057 E
PN G014.4-06.1 0.185 0.054 5610 4558 7251 -601 5.4 0.146 72 S wels
PN G014.8-08.4 0.395 0.055 2654 2378 3050 -392 9 0.116 -24 E O(H)3-4
PN G014.8-25.6 1.512 0.245 731 612 877 -316 32.3 0.114 E
PN G015.4+05.6 0.11 0.031 7808 6529 9766 769 4.5 0.17 R
PN G015.4-04.5 0.225 0.053 4957 4173 6409 -397 3 0.072 46 R O(H)3 If
PN G016.4-01.9 0.449 0.017 2226 2154 2309 -77 5.9 0.063 29 R O(H)7I(fc)
PN G016.9-09.7 0.368 0.058 2896 2465 3428 -488 29 0.407
PN G017.3-21.9 0.699 0.039 1424 1360 1494 -533 59.5 0.411 13 E O(H) + ?
PN G017.6-10.2 0.584 0.032 1761 1662 1865 -313 29.6 0.252 3 R O(H)3-5Vz
PN G019.8-23.7 0.863 0.19 1184 985 1420 -477 139.5 0.8 R
PN G020.3-06.9 0.228 0.022 4471 4118 4973 -543 11 0.238
PN G020.7-05.9 0.294 0.028 3538 3268 4071 -368 3.5 0.06 46 R O(H)4-8III
PN G020.7-08.0 0.754 0.066 1364 1253 1487 -191 105 0.694 B O(H)3-5Vz
PN G021.4+02.5 0.161 0.035 6018 4973 6929 270 30 0.875 R
PN G022.9+22.7 1.125 0.131 906 800 1050 351 180 0.791 A
PN G025.3+40.8 0.434 0.048 2294 2074 2595 1500 7.5 0.083 22 E O(H)5f
PN G025.4-04.7 0.649 0.068 1639 1449 1853 -135 49.8 0.395 -13 E hgO(H)
PN G026.0+46.6 0.338 0.04 2949 2617 3537 2144 60 0.858
PN G026.1-17.6 1.018 0.015 983 970 999 -298 247.5 1.179 A
PN G026.5-03.0 0.264 0.078 4464 3528 5498 -220 2.2 0.048
PN G027.4-03.5 0.209 0.058 4873 4077 5859 -298 7.5 0.177 47 R
PN G027.6+16.9 0.593 0.044 1692 1568 1804 492 55 0.451 R sdO
PN G029.2-05.9 0.33 0.047 3077 2716 3509 -319 11.8 0.176 -43 E [WO 4]
PN G029.3-01.2 0.781 0.061 1303 1203 1399 -28 29.3 0.185 B
PN G030.5-18.4 7.763 0.064 129 128 130 -41 1350 0.844 DA
PN G030.8+03.4a 1.921 0.268 546 493 628 33 S
PN G031.0-10.8 0.254 0.076 4216 3425 5268 -797 3.5 0.071 48 E
PN G032.1-06.2 8.06 0.038 124 124 125 -14 600 0.361
PN G033.1-06.3 1.13 0.193 1001 835 1249 -111 37.9 0.184 0 B
PN G034.1-10.5 0.553 0.072 1821 1618 2045 -332 39.5 0.349 R hgO(H)
PN G034.6+11.8 0.572 0.071 1788 1609 1991 367 7 0.061 -9 B Of-WR(H)
PN G034.7-06.2 0.209 0.027 4765 4335 5238 -520 7.8 0.179 R
PN G035.7+19.2 0.313 0.057 3299 2807 4026 1085 26.3 0.42 E

Notes. Full table is available at CDS.

References. Angular radii < R> ang and morphological types taken from HASH database. Radial velocities Velrad taken from Simbad database. Spectral types taken from Weidmann et al. (2020).

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