Table 1
Compact PNe presented in this paper.
| Name (Alias) | RA (J2000.0) | Dec (J2000.0) | Rphot [″] (HST) | Density [arcmin−2] | References / Comments |
|---|---|---|---|---|---|
| PN G061.9+41.3 (DdDm-1) | 16:40:18.20 | +38:42:19.9 | 0.6(a) | 1.3 | Henry et al. (2008) |
| PN G025.3−04.6 | 18:54:20.04 | −08:47:32.9 | 0.48 | 53.4 | Stanghellini et al. (2016) |
| PN G042.9−06.9 | 19:34:33.54 | +05:41:03.0 | 0.48 | 23.0 | Stanghellini et al. (2016) |
| PN G205.8−26.7 | 05:03:41.85 | −06:10:03.0 | 1.04 | 1.8 | Stanghellini et al. (2016) |
| PN G295.3−09.3 | 11:17:43.16 | −70:49:32.2 | 0.48 | 12.6 | Stanghellini et al. (2016) |
| PN G334.8−07.4 | 17:03:02.86 | −53:55:54.0 | 0.44 | 25.1 | Stanghellini et al. (2016) |
| PN G004.8−22.7 (He2–436) | 19:32:06.69 | −34:12:57.8 | >0.21 | 4.6 | Zijlstra et al. (2006) |
| LMC-SMP-25 | 05:06:24.00 | −69:03:19.2 | 0.23 | 68.4 | Shaw et al. (2001) |
| LMC-SMP-31 | 05:09:20.23 | −67:47:25.2 | 0.15 | 44.6 | Shaw et al. (2001) |
| LMC-SMP-53 | 05:21:32.93 | −67:00:05.5 | 0.40 | 19.6 | Shaw et al. (2001) |
| LMC-SMP-58(b) | 05:24:20.81 | −70:05:01.9 | 0.13 | 91.8 | Shaw et al. (2001) |
| LMC-Sa-104a | 04:25:32.18 | −66:47:16.3 | <0.13 | 1.9 | Shaw et al. (2006) |
| SMC-SMP-1 | 00:23:58.67 | −73:38:03.8 | 0.15 | 4.4 | Stanghellini et al. (2003) |
| SMC-SMP-2 | 00:32:38.81 | −71:41:58.7 | 0.25 | 1.8 | Shaw et al. (2006) |
| SMC-SMP-8 | 00:43:25.30 | −72:38:18.9 | 0.40 | 17.4 | Stanghellini et al. (2003) |
| SMC-SMP-13 | 00:49:51.71(c) | −73:44:21.3 | 0.20 | 24.0 | Stanghellini et al. (2003) |
| SMC-SMP-18 | 00:51:57.97 | −73:20:31.1(d) | 0.14 | 58.3 | Stanghellini et al. (2003) |
| SMC-SMP-20 | 00:56:05.39 | −70:19:24.7 | 0.20 | 2.2 | Stanghellini et al. (2003) |
| SMC-SMP-24 | 00:59:16.09 | −72:01:59.7 | 0.38 | 25.9 | Stanghellini et al. (2003) |
| SMC-SMP-25 | 00:59:40.51(e) | -71:38:15.1(e) | 0.19 | 12.8 | Stanghellini et al. (2003) |
| STRIPE82-0130 | 22:03:15.14 | +01:17:20.9 | – | N/A | Transient, not a PN |
Notes. All PNe listed here are included in our line atlas and are available as a part of our data pack available at the CDS. (a)From a 1993 archival HST image, after deconvolution to correct for spherical aberration. (b)Used as a wavelength calibration source for JWST (Jones et al. 2023); most likely too crowded for Euclid calibration purposes. (c)Incorrectly typed in Stanghellini et al. (2003). (d)Shifted ~1″ south by us based on the ESO finding chart tool using the Gaia catalogue display. (e)Wrong coordinates in Stanghellini et al. (2003), corresponding to LMC-SMP-71 in Shaw et al. (2001). We used the coordinates from Meyssonnier & Azzopardi (1993), adjusted to higher precision.
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