One star, two star, red star, blue star: an updated planetary nebula central star distance catalogue from Gaia EDR3
AAstronomy & Astrophysics manuscript no. aanda © ESO 2021March 1, 2021
One star, two star, red star, blue star: an updated planetary nebulacentral star distance catalogue from
Gaia
EDR3
N. Chornay and N. A. Walton
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdome-mail: [email protected] , e-mail: [email protected]
February 2021
ABSTRACT
Aims.
Planetary nebulae (PNe) are a brief phase of stellar evolution and as such some of the rarest objects in our galaxy. Accurateidentification of PN central stars (CSPNe) in large surveys such as
Gaia is key to exploiting the scientific potential of those surveysfor the study of PNe and stellar evolution.
Methods.
We apply our automated search method to identify source detections corresponding to CSPNe and compact PNe in therecently released
Gaia
Early Data Release 3 (EDR3). The method is updated to incorporate photometric uncertainties.
Results.
The new catalogue o ff ers improved completeness and accuracy over the previous one, and will continue to be valid forthe upcoming Gaia
Data Release 3 (DR3). The identification of EDR3 sources unlocks the improved astrometry and photometrystemming from calibration updates and a longer mission duration, even for sources that have previously been identified.
Key words. planetary nebulae: general – Catalogs – Methods: statistical
1. Introduction
Planetary nebulae (PNe) represent a brief but enigmatic stage inthe evolution of low- and intermediate-mass stars towards theends of their lives. PNe and in particular central stars of PNe(CSPNe) are some of the rarest objects observed by
Gaia (GaiaCollaboration et al. 2016), a European Space Agency (ESA) mis-sion conducting precision astrometry and photometry for nearlytwo billion sources in the Milky Way and beyond.
Gaia showsgreat potential for the study of PNe: parallaxes are indicative ofdistances and in turn CSPN absolute magnitudes and evolution-ary phase; proper motions add another dimension to dynamicsand relate PNe to their parent stellar populations, constrainingages and masses; and finally, repeated photometric observationscontribute to study of variability and binarity.Unlocking the potential of
Gaia requires accurately match-ing Gaia sources to PN central stars, that is, finding some of therarest needles in the
Gaia haystack. This was the aim of our firstpaper (Chornay & Walton 2020), in which we used an e ffi cient,automated approach to generate the most complete and accuratecatalogue of CSPNe in Gaia
Data Release 2 (DR2, Gaia Collab-oration et al. 2018).In this work we present a new catalogue of PN central starsand compact PNe in
Gaia
Early Data Release 3 (EDR3, GaiaCollaboration et al. 2020) based on the same methodology. Thecatalogue will remain valid for Data Release 3 (DR3) expectedin 2022, and thus provide a valuable resource for the study ofgalactic PNe in for several years to come. In Sect. 2 we discussthe relevant changes to the
Gaia
EDR3 data, and their impli-cations for the matching algorithm and the use of the resultingcatalogue. In Sect. 3 we highlight some changes relative to theDR2 catalogue, and discuss the detection limits of
Gaia as theyrelate to binarity and nebula characterisation.
2. Methods
Our planetary nebula input catalogue is once again the latest ver-sion of Hong Kong / AAO / Strasbourg H α (HASH) PN catalogue(Parker et al. 2016, as of ). Driven by new discoveries and spec-troscopic confirmation, the catalogue has grown to 2623 ‘true’(spectroscopically confirmed) PNe (up 6%) and to 3710 PNeoverall (including ‘likely’ and ‘possible’ PNe, up 4%). We ob-served in our DR2 work that a few extremely extended nebu-lae had o ff set CSPN that would otherwise be outside of our 60 (cid:48)(cid:48) search radius. With the aim of increasing the usefulness of theresulting catalogue, we adopt positions for Sh 2-188 from Wei-dmann & Gamen (2011) and for FP J1824-0319 and FP J0905-3033 from Parker et al. (2006). Gaia
EDR3 is likewise larger than DR2. It covers an addi-tional 12 months of data collection, for a total of 34 months.The longer survey duration along with significant improvementsto calibration results in better completeness (7% more sourcesoverall) and higher astrometric precision (particularly propermotions). In addition to the increased number of sources, thesource IDs in EDR3 do not necessarily correspond to those in inDR2. The set of sources in EDR3 will be the same for the fullDR3 expected in 2022, which will include additional data prod-ucts, such as new radial velocities, variable source classificationsalong with epoch photometry, and low-resolution spectra.EDR3 contains several new columns. Particularly relevant toPNe are a couple of statistics related to image parameter determi-nation (IPD, Lindegren et al. 2020), the processing step involv-ing fitting a point or line-spread function to the
Gaia
CCD data.The first is ipd_gof_harmonic_amplitude : a strong depen-dence of the goodness of fit on the scan angle suggests a sourcethat is elongated, suggesting a partially resolved binary or an ex-tended source such as a galaxy or a distant, compact PN. The
Article number, page 1 of 32 a r X i v : . [ a s t r o - ph . S R ] F e b & A proofs: manuscript no. aanda second is ipd_frac_multi_peak : multi-peak detections indi-cate a likely close binary, though depending on the separationit may only be resolved in some directions (as for all but thebrightest sources
Gaia ’s imaging is only in a single dimension).The resolution has also improved. In DR2 sources were com-bined (with the duplicated_source set) when separated byless than 0.4 (cid:48)(cid:48) ; the minimum separation in EDR3 has been re-duced 0.18 (cid:48)(cid:48) , though incompleteness starts below 1.5 (cid:48)(cid:48) and isquite severe below 0.7 (cid:48)(cid:48) (Fabricius et al. 2020).Finally phot_bp_rp_excess_factor is no longer used asa filter for published photometry (as it was in DR2, Evans et al.2018), so more sources have published G BP – G RP colours. Ex-cess factor is particularly relevant for PNe: while they can su ff erfrom the same crowding issues that other sources do, their ex-tended structure and bright emission lines (as noted by Rielloet al. 2020) can also lead to disagreements between the fluxes inthe G band and those in G BP and G RP . We use the matching approach employed in Chornay & Wal-ton (2020) and point the reader to that work for more detailson the method, recalling here the salient ideas and discussingthe changes made. The aim is to match PN central stars orcompact / stellar-like nebulae to Gaia sources in order to exploitthe
Gaia astrometry and photometry. The expectation is thatthese sources will be close to the catalogued position of thePN, but the possibility of non-detections, spurious backgroundsources, and positional inaccuracies necessitates a more nuancedapproach than the simple nearest-neighbour matching. Manualmatching is time-consuming, with poorly characterised uncer-tainties, and secure identification anyway requires spectroscopyand / or high resolution imagery with good coverage towards theUV, which is not available for much of the sky.The probabilistic approach taken by likelihood ratio methodof Sutherland & Saunders (1992) is well-suited to addressingsome of these issues. The idea is to compare the probabilityof finding a true match at an angular separation r to finding aspurious match at that separation, given the positional distribu-tions distribution of true matches P ( r | genuine) and P ( r | chance).In our implementation we assume a uniform background den-sity in each field, and a radially symmetric positional distribu-tion of true central stars parameterised by the radius of the PN(allowing larger PNe to have more o ff set central stars). We alsoemploy the colour distributions of true CSPNe and backgroundsources, parameterised based on the photometric excess factor,with the e ff ect of down-weighting colours for sources whosecolour is potentially contaminated by nearby sources or back-ground. The distributions are derived iteratively, using sourceswith secure identifications based on colour to empirically deter-mine the positional distribution of true central stars, and in turnusing the positionally secure sources to update the colour dis-tribution. This works because CSPNe are often much bluer thantypical Gaia sources and therefore can be selected purely basedon colour with relatively high confidence.We have made a couple of small changes to the matching al-gorithm in the treatment of the G BP – G RP colours. In deriving theinitial and final colour distributions, we only considered sourceswith G brighter than 19. Then in computing the likelihood ratiosfor individual sources we convolved the densities with the photo-metric uncertainties, after accounting for the smoothing alreadyapplied by the kernel density estimation. This change lessens theimpact of faint sources with extreme and likely spurious colours.We also adopted the prescription of Riello et al. (2020) for de- Fig. 1: Reliability of Gaia
DR2 source matches versus the newEDR3 source matches for ‘true’ PN present in both works. Redpoints are objects where the location of the match has changedby more than 0.1 (cid:48)(cid:48) , indicating that a (likely) di ff erent object hasbeen identified as the best match (as opposed to the same objectbeing assigned a di ff erent identifier).scribing a locus of photometric excess values of well-behavedsources, replacing the perscription from Evans et al. (2018).
3. Results
The resulting distribution of reliabilities is for the most part un-changed. A comparison with the catalogue from DR2 is shownin Fig. 1. Most objects are have reliability within 0.1 of theirprevious value, except in the case of new detections changingthe best match.The full catalogue of the 2118 highest ranked matches withreliability > ω indicating par-allax. Fig. 2 shows wide- and narrow-band imagery from the VPHAS + survey (Drew et al. 2014) overlayed with Gaia
EDR3 sources fora small selection of PNe. Data from VPHAS + were not used aspart of the matching, but the images provide good examples ofsome of the changes encountered in the updated Gaia data.KFL 16 and BMP J0713-0432 both have new detections inEDR3 that were not present in DR2. The CSPN of KFL 16 hasno
Gaia colour but is su ffi ciently central that it is selected byour method; its blue colour is evident in the VPHAS + imagery.The CSPN of BMP J0713-0432 does exhibit a blue G BP – G RP colour and as such is selected despite not being the closest to thenominal position of the PN.NGC 2440 had a clear central star detection in DR2; the pres-ence of many new nebular detections in EDR3 dilutes the cer-tainty of that match, both through providing alternate candidatesand through increasing in the density of background sources. More colours help to separate intrinsic colour and reddening e ff ects,but uniform photometric calibration, particularly in the u (cid:48) band, is di ffi -cult. Sky coverage is also limited.Article number, page 2 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from Gaia
EDR3
Fig. 2: VPHAS + images of (from top to bottom) KFL 16, BMPJ0713-0432, NGC 2440, and Msc 1-12, centred on their coordi-nates from HASH. North is up and east is to the left. The colourimages in the first two columns are r (cid:48) / g (cid:48) / u (cid:48) and H α / r (cid:48) / i (cid:48) , whichcapture stellar colours and nebula emission. The third and fourthimage columns are quotient ( r (cid:48) – H α ) images overlayed with Gaia detections from
Gaia
DR2 and
Gaia
EDR3 respectively.The true CSPN is still selected (it is overwhelmed by the neb-ula in the VPHAS + imagery but clear in HST imagery), but withreduced confidence. In the case of Msc 1-12, the lone detectionfrom DR2 has disappeared, and no matching EDR3 source isfound. Several CSPNe are visual binaries in
Hubble
Space Telescope(HST) imagery: ten are presented in Ciardullo et al. (1999)("probable associations") as well as additional pairs in Benettiet al. (2003) and Liebert et al. (2013). Typical separations of theknown pairs are fractions of an arcsecond; with the improvedresolution of
Gaia
EDR3 we expect that more of these will beresolved. The detections for these PNe are listed in Table 1.Abell 33 and NGC 3132 have companions at wide separa-tions detectable from the ground (though the catalogue positionof NGC 3132 is actually closer to that of the companion star,leading to ambiguity in our matching results). Of the closer pairs,only K 1-22 is resolved into separate sources by
Gaia , possiblyon account of their similar magnitudes. Another four PNe havea notable fraction of multi-peak detections, while the remainingPNe seem to have companions that are either too faint (e.g. Abell31 and K 1-27) or too close (e.g. NGC 6818). Though not in thetable, the harmonic amplitudes are smaller than those of nebuladetections (typically between 0.01 and 0.1; the largest is 0.26 forNGC 6818, the closest pair in the sample), and the re-normalisedunit weight error (RUWE, indicative of excess astrometric error;Lindegren 2018) values range from normal to significant. Noneare duplicated sources. Table 1:
Gaia detections of known close visual binaries.PN Sep. a ∆ V b Rel. c G Mul. d RUWE( (cid:48)(cid:48) ) (mag) (mag) (%)Abell 31 0.26 > e . . . e e -5.7 f Notes.
Rows with first columns blank indicate the
Gaia -detected com-panion of the (assumed PN progenitor) in the row above. Single rowsindicate that
Gaia has not resolved the pair. ( a ) Literature separation, ex-cept where noted. Most values are from Ciardullo et al. (1999), exceptfor EGB 6 (Liebert et al. 2013) and NGC 6818 (Benetti et al. 2003). ( b ) Di ff erence in HST V magnitude between ionising star and compan-ion (a positive di ff erence indicates companion is fainter). ( c ) Reliability. ( d ) IPD multipeak fraction. ( e ) Gaia value, within 0.02 (cid:48)(cid:48) of literature HSTvalue. ( f ) The ionising star of NGC 3132 is thought to be the fainter ofthe pair, so highest reliability match here is not correct in that sense.
About 175 highest ranked potential matches (reliability > < (cid:48)(cid:48) ). Of the ∼
60 PN with at least two potential matches (wherethe second highest reliability is > < (cid:48)(cid:48) separation). These likely include some genuine binary sys-tems, though their blended colour photometry and degraded as-trometry makes it di ffi cult to characterise the companion star andsecure its relation through e.g. proper motion comparison. During the initial 28 days of the
Gaia mission, in which theecliptic-poles scanning law was employed, there were many neb-ula detections for the high-declination PN NGC 6543 (Fabriciuset al. 2016). These were not present as sources in the first twodata releases: only the central 11th magnitude star was included.Now in EDR3 we once again see nebula detections (Fig. 3,left; c.f. Fig. 14 in Fabricius et al. 2016), though all are two-parameter solutions, lacking proper motions that would facilitatestudies of the nebular dynamics. NGC 6543’s previously mea-sured expansion rate of 3 . ± .
16 mas yr − (similar to otherPNe; Schönberner et al. 2018) would be easily detectable forstars of similar brightness, but centroiding di ffi culty caused bythe extended nature of the nebula detections means that the posi-tional uncertainty is much larger than the positional changes dueto a few years of proper motion. The positional uncertainties dotrace the features, tending to be smaller in the radial direction.Several other nebulae in the New General Catalogue (whichtend to be bright and nearby) have Gaia nebula detections.Counting sources within the PN radius with corrected excess Also featured as
Gaia ’s image of the week: . Article number, page 3 of 32 & A proofs: manuscript no. aanda
Fig. 3:
Hubble narrowband images of NGC 6543 (left) and thecentral region of NGC 5189 (right) overlayed with
Gaia
EDR3sources (blue points and crosses). Errorbars have been rotated toreflect the direction of the principle component of the covariancematrices, and are greatly exaggerated for visibility (with di ff er-ent scales in each plot). Gaia source locations have been shiftedto align the central star detection with the central star location inthe HST image. North is up and east to the left for NGC 6543,while the orientation of NGC 5189 is rotated 90 ◦ so that north isto the left. (Images: Hubble
Legacy Archive / ESA / NASA.)factor >
20 and IPD goodness of fit harmonic amplitude > − . ), NGC 2440 and NGC 6302 have the most (38 and 35 re-spectively); others with more than 10 detections are NGC 2392,NGC 40, and NGC 5189 (shown in Fig. 3, right).
4. Conclusions
We have presented an updated version of our CSPN cataloguefor
Gaia
EDR3. The minimal changes required demonstrate therobustness of our original method.
Gaia
DR3, expected in 2022,is based on the same astrometric and photometric data as
Gaia
EDR3, so the astrometry from this release will be the best avail-able for studying PN based on their distances and kinematics un-til the next full
Gaia data release in several years to come.
Gaia
DR3 will o ff er new low-resolution spectroscopy, which can beused as an improved (but more complicated) selection parame-ter. More independent colour dimensions will provide the possi-bility to separate intrinsic colour and reddening for CSPNe, andpotentially even to identify emission-line objects, while main-taining the advantage relative to ground-based surveys of moreuniform calibration and sky coverage. Acknowledgements.
This research has made use of data from theEuropean Space Agency (ESA) mission
Gaia ( ), processed by the Gaia
Data Processing and Analy-sis Consortium (DPAC; ). Funding for the DPAC has been provided by national institu-tions, in particular the institutions participating in the
Gaia
Multilateral Agree-ment. This research has also made use of the HASH PN database ( http://hashpn.space ), of Astropy ( ), a community-developed core Python package for Astronomy (Astropy Collaboration et al.2013; Price-Whelan et al. 2018), and of "Aladin sky atlas" developed at CDS,Strasbourg Observatory, France. Parts of this research were based on data prod-ucts from observations made with ESO Telescopes at the La Silla Paranal Ob-servatory under programme ID 177.D-3023, as part of the VST Photometric H α Survey of the southern Galactic plane and bulge (VPHAS + , ).This research was supported through the Cancer Research UK grant A24042. References
Astropy Collaboration, Robitaille, T. P., Tollerud, E. J., et al. 2013, A&A, 558,A33Benetti, S., Cappellaro, E., Ragazzoni, R., Sabbadin, F., & Turatto, M. 2003,A&A, 400, 161Chornay, N. & Walton, N. A. 2020, A&A, 638, A103Ciardullo, R., Bond, H. E., Sipior, M. S., et al. 1999, AJ, 118, 488Drew, J. E., Gonzalez-Solares, E., Greimel, R., et al. 2014, MNRAS, 440, 2036Evans, D. W., Riello, M., De Angeli, F., et al. 2018, A&A, 616, A4Fabricius, C., Bastian, U., Portell, J., et al. 2016, A&A, 595, A3Fabricius, C., Luri, X., Arenou, F., et al. 2020, arXiv e-prints, arXiv:2012.06242Gaia Collaboration, Brown, A. G. A., Vallenari, A., et al. 2018, A&A, 616, A1Gaia Collaboration, Brown, A. G. A., Vallenari, A., et al. 2020, arXiv e-prints,arXiv:2012.01533Gaia Collaboration, Prusti, T., de Bruijne, J. H. J., et al. 2016, A&A, 595, A1Liebert, J., Bond, H. E., Dufour, P., et al. 2013, ApJ, 769, 32Lindegren, L. 2018, GAIA-C3-TN-LU-LL-124Lindegren, L., Klioner, S. A., Hernández, J., et al. 2020, arXiv e-prints,arXiv:2012.03380Parker, Q. A., Acker, A., Frew, D. J., et al. 2006, Monthly Notices of the RoyalAstronomical Society, 373, 79Parker, Q. A., Bojiˇci´c, I. S., & Frew, D. J. 2016, in Journal of Physics ConferenceSeries, Vol. 728, Journal of Physics Conference Series, 032008Price-Whelan, A. M., Sip˝ocz, B. M., Günther, H. M., et al. 2018, AJ, 156, 123Riello, M., De Angeli, F., Evans, D. W., et al. 2020, arXiv e-prints,arXiv:2012.01916Schönberner, D., Balick, B., & Jacob, R. 2018, A&A, 609, A126Sutherland, W. & Saunders, W. 1992, MNRAS, 259, 413Weidmann, W. A. & Gamen, R. 2011, A&A, 526, A6
Article number, page 4 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
Gaia
EDR3
Appendix A: Best matches table
Article number, page 5 of 32 & A proofs: manuscript no. aanda
Table A.1: Best Matches Catalogue
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status (deg) (deg) (mag) (mag) (mas) (mas) (”)116.0-04.8 IPHASXJ000021.4 + + + . . . P117.5 + -5.3 Dr 27 422428519103328128 2.76432 57.17670 1.000 -0.233 17.718 1.008 0.091 270.0 L120.0 + + . . . -0.056 17.840 0.038 0.085 . . . TJ16 4688984022393506432 12.90273 -72.53528 0.998 -0.431 20.411 -0.454 0.628 . . .
T123.0 + + . . . . . . + . . . . . . + -8.9 Dr 36 411078093067339136 16.91690 53.87332 1.000 0.117 18.811 0.851 0.196 81.0 L126.7-15.4 Fr 2-30 401414034397108352 18.32132 47.23320 0.232 2.371 19.360 1.198 0.267 30.0 P127.6-13.5 PaStDr 3 400211958948711552 19.87035 49.01925 1.000 -0.301 13.352 1.240 0.033 360.0 P126.3 + + + + / + + + + + + + + + + + + + + + + . . . . . . + . . . . . . + + + . . . + . . . . . . + + Article number, page 6 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
Gaia
EDR3
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )167.4-09.1 K 3-66 172188296914590208 69.15516 33.65835 0.999 0.902 15.302 0.255 0.128 1.1 T174.2-14.6 H 3-29 147952487953283712 69.34764 25.04414 1.000 0.699 18.220 0.137 0.171 11.9 T165.5-06.5 K 3-67 175182924208301824 69.94965 36.76194 0.909 0.503 17.410 . . . . . . . . .
T158.6 + . . . . . . . . . . . . + + + + + . . . T168.4 + + + + . . . L156.3 + + . . . . . . + . . . T196.6-10.9 NGC 2022 3336140414380977664 85.52579 9.08627 1.000 -0.174 15.707 0.438 0.053 13.9 T200.5-13.1 Kn 63 3320608713128049280 85.52796 4.71742 1.000 -0.012 17.468 0.767 0.095 176.0 T173.5 + + . . . . . . + + + + + . . . . . . + + . . . . . . + . . . T204.0-08.5 Abell 13 3318052348593263488 91.19955 3.94319 1.000 0.209 19.571 -0.002 0.424 85.0 T278.7-28.9 RP 4791 5282784004280482816 92.36173 -68.65654 0.978 0.159 20.206 -0.268 0.372 3.0 T197.8-03.3 Abell 14 3330404266518636416 92.78607 11.77884 0.977 0.764 15.081 0.218 0.029 20.0 T209.1-08.2 PHR J0615-0025 3121659647518519552 93.83483 -0.43044 1.000 0.384 20.181 0.101 0.843 52.0 T208.9-07.8 TaWe 1 3121886520577421568 94.06408 -0.00694 1.000 -0.207 18.573 0.592 0.194 72.5 T158.9 + + . . . . . . + + + . . . . . . + + + . . . P Article number, page 7 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )216.9-05.2 MPA J0639-0554 3100542667721862912 99.99219 -5.91587 0.986 0.224 18.909 -0.068 0.284 2.5 T192.5 + + + + + + + + + + + . . . . . . + + . . . . . . + . . . . . . + . . . . . . + . . . . . . + + + + + . . . . . . . . . + + + + . . . . . . + + + + + + . . . . . . + + . . . . . . + + + . . . + + + + + + + + + Article number, page 8 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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EDR3
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )227.3 + + + + + + + + + + . . . + + . . . . . . + + + + + . . . . . . + . . . . . . . . . + + + . . . . . . + . . . . . . + + . . . . . . + + . . . . . . + + + . . . . . . . . . T275.7-04.9 PHR J0914-5555 5310074162075205248 138.51469 -55.92230 0.980 0.114 16.500 0.108 0.037 14.2 T275.0-04.1 PB 4 5310278598198854016 138.78224 -54.87883 1.000 0.117 16.276 0.191 0.045 6.1 T261.9 + + . . . . . . . . . . . . . . . . . . + + + + . . . . . . . . . . . . + + + + + Article number, page 9 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )162.1 + + + . . . T243.0 + + + + . . . . . . . . . . . . T274.3 + + + . . . . . . + + . . . . . . . . . + + + + + + + . . . . . . + + + + + + . . . + . . . . . . + + + . . . T148.4 + + + + . . . . . . . . . + . . . . . . + . . . . . . . . . + + + . . . . . . + + . . . . . . + + + + + + + . . . . . . . . . . . . . . . . . . . . . + + + + Article number, page 10 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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EDR3
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )144.8 + + + + + + + + . . . . . . . . . . . . + . . . . . . + + . . . . . . . . . . . . P300.2 + + . . . . . . + + . . . . . . . . . . . . + . . . . . . . . . . . . T302.1 + + . . . . . . + + + . . . T304.8 + . . . . . . . . . . . . . . . . . . . . . + + + . . . . . . . . . + + . . . . . . . . . + . . . + . . . . . . + . . . + + + . . . . . . + . . . P318.4 + + + . . . . . . + + + . . . . . . + . . . . . . . . . + Article number, page 11 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )311.4 + + + + + + + + + . . . T310.8-05.9 LoTr 7 5847795443251442304 213.85047 -67.53176 0.997 0.030 19.384 -0.154 0.252 8.0 T308.6-12.2 Hen 2-105 5796437220731788288 213.85311 -74.21281 1.000 -0.231 14.599 0.271 0.032 20.8 T313.3 + . . . . . . + + + . . . . . . . . . T315.9 + + + + . . . . . . . . . T314.4 + + + + + + + + + + . . . + . . . . . . + . . . . . . + . . . + . . . . . . + . . . . . . . . . . . . . . . + + + + + + . . . . . . . . . . . . T320.9 + + . . . . . . + + . . . . . . + . . . . . . + + + + + + . . . . . . P319.3-02.6 BMP J1513-6052 5876220911242751488 228.40182 -60.86768 0.466 0.883 21.146 . . . . . . + + . . . . . . . . . + + + . . . . . . . . . + + Article number, page 12 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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EDR3
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )323.9 + . . . . . . . . . + . . . . . . + + + + + + + . . . . . . + + + + . . . . . . . . . T322.5-05.2 NGC 5979 5833343531156787840 236.92156 -61.21822 1.000 -0.002 16.284 0.263 0.051 10.1 T332.3 + + . . . . . . + + + + + . . . . . . . . . + + + . . . + + . . . . . . + + . . . + . . . T337.0 + + + + . . . . . . + + . . . . . . . . . L345.5 + + + + + . . . . . . . . . . . . P328.2-03.9 BMP J1613-5633 5835460572057022336 243.46524 -56.55452 0.526 . . . . . . . . . + + . . . . . . + . . . . . . . . . Article number, page 13 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )326.0-06.5 Hen 2-151 5831451649598626560 243.92618 -59.90029 0.999 0.481 12.730 0.318 0.136 0.9 T331.7-01.0 Mz 3 5934701559547878144 244.30577 -51.98633 0.982 1.754 13.190 0.366 0.086 23.9 P330.6-02.1 Hen 2-153 5933070468426290944 244.30984 -53.53489 0.626 0.380 20.187 0.973 0.957 9.4 T336.1 + + + + -1.0 DeGaPe 64 5934781415925167104 244.76411 -51.70235 0.909 . . . . . . . . . + + + + + + . . . . . . . . . + + + + + + . . . L047.0 + + . . . . . . + + . . . . . . . . . + + . . . . . . . . . + . . . + + . . . . . . . . . . . . + + + + . . . . . . . . . . . . . . . + . . . . . . . . . . . . . . . + + . . . . . . + + . . . T344.2 + + + + + + + + + + + + . . . . . . + + . . . T338.4-02.0 MPA J1650-4747 5939391388953453696 252.54091 -47.78469 0.972 2.940 20.614 -1.580 1.430 2.5 T333.7-05.9 PHR J1650-5350 5929999193173827456 252.54869 -53.84050 0.405 0.219 12.593 0.241 0.017 12.0 P
Article number, page 14 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )351.9 + + + . . . . . . + . . . . . . . . . T338.5-02.1 Kn 87 5939388502731608704 252.79331 -47.77850 0.770 2.560 20.188 0.374 0.721 1.8 T347.3 + + . . . . . . + . . . . . . . . . + + + + . . . + + + . . . . . . . . . . . . T350.3 + + + . . . . . . + . . . . . . -1.586 0.861 3.5 P343.9 + + . . . + . . . . . . . . . . . . + . . . . . . . . . . . . . . . + + + + . . . T341.0-02.6 Kn 89 5963209701330219136 255.66466 -46.13373 0.911 2.486 18.505 -0.165 0.210 5.0 T338.1-04.8 PHR J1702-4943 5938219382596554240 255.67484 -49.72259 0.731 0.958 20.499 1.787 1.502 23.5 T334.8-07.4 Hen 3-1312 5923760667266961408 255.76195 -53.93168 0.990 0.957 11.110 0.159 0.052 8.0 T351.1 + + + . . . . . . + + . . . . . . + + . . . . . . + . . . . . . . . . . . . . . . T358.0 + + . . . . . . + . . . T336.2-06.9 PC 14 5924318978646258304 256.56150 -52.50016 0.971 -0.017 16.931 0.464 0.224 3.6 T342.9-02.0 Pe 1-8 5963798451140343936 256.59396 -44.21972 0.590 1.015 19.605 0.118 0.354 11.5 T342.7-02.3 MPA J1706-4434 5963598821057669760 256.70565 -44.57624 0.756 2.338 20.009 0.434 0.519 8.0 T011.4 + + . . . . . . . . . . . . T342.9-02.3 WRAY 16-251 5963605319383850624 256.87751 -44.38065 0.984 1.598 21.077 . . . . . . + . . . . . . + + + . . . . . . . . . + . . . T349.5 + . . . . . . . . . + + . . . T345.2-01.2 H 1-7 5965810351256669952 257.61409 -41.88040 0.991 1.351 16.975 0.958 0.095 5.3 T357.2 + + . . . . . . . . . + + . . . . . . . . . T354.0 + + . . . L Article number, page 15 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )334.3-09.3 IC 4642 5923374773032038528 257.93834 -55.40050 1.000 -0.229 15.903 0.243 0.061 12.1 T355.9 + + + . . . . . . . . . + + + + . . . . . . . . . . . . + . . . P075.7 + + + + + + . . . . . . + . . . . . . + . . . . . . . . . . . . T354.8 + . . . T331.3-12.1 Hen 3-1357 5915762510400725760 259.08777 -59.48987 0.984 0.317 15.355 -3.501 0.746 2.0 T352.7 + . . . . . . . . . L356.7 + . . . P357.3 + + + . . . L355.8 + . . . . . . . . . + + + . . . . . . + + . . . T341.8-05.6 Kn 93 5951003846646334464 259.85803 -47.26345 0.481 0.859 18.545 -0.854 0.187 6.0 T001.9 + + . . . . . . + + . . . . . . . . . + . . . + . . . . . . . . . . . . . . . + . . . . . . + + + + . . . . . . . . . + + + + . . . . . . . . . L349.3-01.1 NGC 6337 5972577055062637056 260.56530 -38.48383 0.904 0.387 15.624 0.594 0.039 23.8 T358.7 + . . . + + + + . . . . . . + . . . . . . + + + . . . . . . . . . + . . . . . . + . . . . . . + + . . . . . . + + + + + + Article number, page 16 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )345.0-04.9 Cn 1-3 5952577144700811136 261.55130 -44.19043 0.989 0.394 13.566 -0.333 0.228 1.0 T352.6 + + + + . . . . . . + + . . . . . . . . . . . . . . . . . . + + + + + . . . . . . + + + . . . P357.3 + + + + + . . . . . . + + + . . . . . . . . . + + + . . . . . . . . . + . . . . . . + . . . . . . + . . . . . . + + . . . + . . . . . . . . . . . . T000.3 + + . . . . . . + + + . . . . . . + + . . . P356.5 + . . . T358.4 + + + + + . . . . . . . . . + + + . . . T359.0 + . . . P349.2-03.5 H 2-14 5961654029849113728 263.08368 -39.85629 0.915 0.780 18.162 0.362 0.175 7.0 T350.8-02.4 H 1-22 5962119947915694976 263.09229 -37.95661 0.993 1.535 18.024 0.678 0.197 1.8 T346.2-05.5 Kn 103 5958481320307081472 263.13916 -43.49477 1.000 0.116 18.858 0.052 0.245 18.0 T348.5-04.0 Kn 109 5959362063504880000 263.16821 -40.74954 0.363 0.325 20.675 . . . . . . + . . . . . . + . . . . . . . . . + . . . + . . . . . . . . . P007.3 + . . . . . . . . . + . . . . . . . . . . . . P000.3 + . . . . . . . . . + + + + . . . . . . . . . + + . . . + . . . . . . + + Article number, page 17 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )356.9 + . . . . . . + . . . . . . + . . . . . . + . . . . . . . . . + + . . . + . . . . . . . . . + + + . . . + . . . . . . . . . + + + + . . . . . . + + + . . . . . . . . . + + + . . . . . . . . . . . . P005.2 + + . . . . . . + . . . . . . + + . . . . . . + + + + + + . . . . . . . . . . . . . . . T002.1 + + + . . . . . . . . . . . . . . . . . . + . . . L007.0 + + + + + + + + . . . . . . . . . + . . . . . . . . . + + . . . . . . . . . + + . . . . . . + . . . . . . . . . + . . . . . . . . . + . . . . . . . . . . . . . . . . . . + + . . . . . . . . . P004.1 + + + . . . T027.6 + + . . . + + Article number, page 18 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )355.2-02.0 PPA J1741-3405 4053444556158195712 265.49614 -34.09294 0.447 1.890 20.020 -1.024 0.636 3.2 T010.7 + + . . . . . . . . . + . . . + + + + . . . . . . . . . . . . . . . . . . . . . T002.6 + + . . . + . . . . . . . . . . . . + + + . . . . . . + . . . + + + + . . . . . . . . . + + . . . . . . . . . . . . . . . + . . . P003.9 + . . . . . . + . . . . . . . . . . . . . . . . . . + . . . . . . P005.1 + + + . . . . . . + + . . . + . . . . . . . . . . . . . . . + . . . . . . . . . + . . . L301.8 + . . . P001.7 + . . . . . . . . . . . . . . . + + + + + . . . + . . . . . . + + . . . . . . . . . . . . + . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . + + + + . . . . . . . . . + . . . . . . L007.7 + . . . . . . . . . Article number, page 19 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )355.0-03.7 K 5-18 4041450327354434304 267.12329 -35.09133 0.939 -0.954 19.621 -0.188 0.785 5.5 T004.1 + + . . . + . . . . . . + + + . . . . . . . . . + + . . . . . . . . . + + . . . . . . . . . + . . . + . . . + . . . . . . + . . . . . . . . . + . . . P355.5-03.7 PHR J1749-3438 4041487500447313152 267.49522 -34.64403 0.312 . . . + + + + . . . . . . . . . . . . . . . . . . . . . T009.3 + . . . . . . . . . P356.2-03.6 PPA J1751-3401 4041669950493674240 267.77879 -34.02818 0.676 . . . . . . . . . . . . . . . . . . + . . . . . . . . . . . . P358.9-02.1 PHR J1751-3059 4055764285137097728 267.91158 -30.99831 0.934 . . . . . . . . . + . . . . . . . . . . . . . . . + . . . P358.0-02.7 PN Al 2-O 4043622756199128064 267.93871 -32.05112 0.617 2.354 16.020 0.152 0.063 4.5 T010.1 + . . . + . . . . . . . . . . . . T010.4 + . . . . . . + . . . . . . . . . T009.4 + . . . . . . T355.4-04.3 K 5-34 4040802611953843584 268.09613 -35.07160 0.809 . . . . . . . . . + . . . . . . + . . . . . . + Article number, page 20 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )356.0-04.2 PHR J1753-3428 4041594668305141888 268.27046 -34.47757 0.936 . . . . . . . . . . . . . . . . . . . . . . . . . . . + . . . + . . . . . . + . . . . . . . . . . . . . . . + . . . + . . . . . . + . . . . . . . . . . . . . . . . . . . . . . . . + + . . . . . . . . . + + . . . . . . . . . P359.3-03.1 M 3-17 4044076167334983808 269.10688 -31.07147 0.593 1.389 16.231 0.195 0.062 1.4 T359.2-03.1 PHR J1756-3112 4044074140098515840 269.12009 -31.21073 0.840 . . . . . . . . . + . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . + + . . . P356.7-04.8 H 1-41 4042368312133298816 269.32961 -34.16359 0.900 0.155 16.261 0.262 0.088 6.0 T357.2-04.5 H 1-42 4042401439317575168 269.35488 -33.59532 0.857 0.119 16.495 . . . . . . + . . . P355.4-05.7 MPA J1757-3547 4040485952573587456 269.49820 -35.79939 0.206 . . . . . . . . . . . . . . .
P359.4-03.4 H 2-33 4044019130131217408 269.55225 -31.13511 0.774 1.040 18.843 -0.894 0.407 3.9 T357.1-04.7 H 1-43 4042380857826322176 269.56016 -33.79381 0.955 0.996 14.986 0.571 0.061 1.0 T015.4 + + . . . . . . . . . + . . . . . . . . . . . . + + . . . . . . . . . . . . . . . P358.5-04.2 H 1-46 4043695079072981248 269.76046 -32.36209 0.936 0.991 15.125 -0.447 0.242 1.5 T008.8 + . . . P003.6-01.3 PHR J1759-2630 4064023026181980032 269.80029 -26.50687 0.404 2.007 18.942 0.512 0.273 2.1 T000.5-03.1 KFL 1 4056241095169816448 269.81499 -30.04636 0.869 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . L Article number, page 21 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )354.3-06.8 K 5-38 4037053105525701248 270.01825 -37.28365 0.656 -0.059 18.804 0.345 0.301 . . .
L010.6 + + . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . P340.4-14.1 Sa 1-6 6701733382321164928 270.24781 -52.73889 0.995 0.358 15.969 0.123 0.048 5.5 T002.2-02.5 KFL 2 4062681793803938688 270.24907 -28.27195 0.884 . . . . . . . . . + . . . + . . . . . . . . . . . . P004.3-01.4 PPA J1801-2553 4064173590585927296 270.32875 -25.88918 0.995 2.600 18.735 0.057 0.307 3.0 T357.9-05.1 M 1-34 4042471361358211584 270.34250 -33.29547 0.540 . . . . . . . . . + . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . . . . . . . + . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . . . . . . . . . . + . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . + . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . . . . . . . . . . + . . . L000.6-04.5 PN PM 1-206 4049944565824708608 271.30196 -30.70368 0.934 . . . + . . . . . . . . . . . . . . . + + . . . . . . . . . . . . . . . . . . Article number, page 22 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )004.1-03.0 PHR J1806-2652 4063268348965374976 271.73353 -26.88170 0.284 1.858 18.804 . . . . . . + . . . . . . . . . . . . + + + + . . . . . . . . . . . . . . . . . . . . . + . . . P015.8 + . . . P000.9-05.4 PN PM 1-214 4049234869657862656 272.40835 -30.81458 0.952 0.146 17.469 0.428 0.114 . . .
P001.8-05.0 PHR J1809-2952 4050066203563096704 272.44551 -29.88147 0.518 . . . . . . . . . . . . . . . . . . . . . . . . . . .
P003.3-04.4 PPA J1810-2813 4050871767612742400 272.65051 -28.22945 0.399 . . . . . . . . . . . .
T001.2-05.6 PHR J1811-3042 4049240298544263936 272.76129 -30.70329 1.000 0.346 18.610 0.667 0.422 16.0 T002.7-04.8 M 1-42 4050550916418916864 272.77079 -28.98309 0.735 0.595 18.318 -1.359 0.524 6.5 T009.4-01.2 PHR J1811-2123 4093854116675316096 272.79436 -21.38733 0.586 . . . . . . . . . . . . . . . . . . + . . . T358.3-07.3 SB 52 4039592182712537728 272.91656 -34.00643 0.267 0.438 18.801 -0.226 0.402 7.8 T011.7 + . . . . . . + + . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . . . . + . . . P359.8-07.2 M 2-32 4045707288433971072 273.71084 -32.61535 0.992 -0.422 15.608 -0.052 0.065 4.0 T008.6-02.6 MaC 1-11 4090483254575155968 273.71210 -22.73209 0.925 1.368 17.855 0.089 0.188 4.2 T009.0-02.4 PHR J1814-2220 4090688343507223040 273.73404 -22.34339 0.844 0.581 19.686 -0.227 0.469 6.5 T002.0-06.2 M 2-33 4049596604655713664 273.77735 -30.25927 0.972 0.136 14.739 0.241 0.042 2.7 T011.0-01.3 Pa 98 4094436269390784768 273.77896 -19.99200 0.202 2.416 17.299 0.370 0.111 5.5 P008.4-02.8 PHR J1815-2300 4066445039812849408 273.80423 -23.01804 0.466 . . . + + . . . . . . Article number, page 23 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )359.9-07.4 SB 56 4045704990671786112 273.88528 -32.63350 0.540 0.738 17.375 0.170 0.125 3.0 P014.2 + + . . . . . . . . . L010.0-02.0 MPA J1815-2113 4090916943199396864 273.90406 -21.22260 0.910 2.151 19.528 0.604 0.407 4.0 T354.7-10.0 SB 41 6727598809253337088 273.91268 -38.46570 1.000 0.018 18.369 0.363 0.197 12.9 T005.9-04.2 Pa J1815.7-2551 4064703173079013632 273.94833 -25.85449 0.930 . . . . . . . . . . . . + . . . P021.0 + . . . + . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . + . . . . . . + . . . T020.4 + + + . . . + + . . . . . . + . . . + + . . . . . . . . . T008.2-04.8 M 2-42 4089296950179444864 275.63368 -24.15770 0.966 0.316 17.233 0.055 0.134 1.9 T002.3-07.8 M 2-41 4046378407157239040 275.64371 -30.72481 0.611 0.630 18.810 -0.423 0.210 7.0 T012.6-02.7 M 1-45 4096032936429271296 275.78326 -19.28485 0.929 1.469 16.070 0.107 0.059 4.5 T003.3-07.5 KFL 19 4050998383326315264 275.78719 -29.72386 0.994 -0.036 17.703 0.070 0.111 3.9 T032.9 + + . . . + + + . . . + . . . L034.5 + + + . . . . . . . . . T Article number, page 24 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )043.3 + + + . . . . . . . . . . . . . . . + . . . T017.2-01.7 MPA J1828-1441 4104039335228566528 277.12742 -14.68955 0.569 1.791 18.835 -0.353 0.227 2.5 T022.5 + + . . . T065.4 + + . . . . . . . . . . . . . . . + . . . . . . . . . T004.9-08.6 PPA J1831-2849 4048484315507463296 277.79654 -28.82046 0.995 0.162 17.922 -0.145 0.152 2.2 L055.4 + + . . . + + + . . . + + . . . . . . . . . + . . . . . . . . . . . . . . . + + + . . . . . . + . . . P002.8-10.7 PHR J1835-3135 4046697815310010752 278.89035 -31.59580 0.980 0.020 19.360 0.726 0.311 7.5 T004.6-09.9 SB 9 4047457234247111936 278.92633 -29.63972 0.987 . . . . . . . . . + . . . T016.0-04.3 M 1-54 4099764713235026688 279.03483 -16.99918 0.996 . . . . . . . . . + . . . . . . + + . . . L027.5 + . . . . . . . . . . . . . . . + Article number, page 25 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )004.0-11.1 M 3-29 4047152806963235584 279.85756 -30.67704 0.991 -0.173 15.419 0.169 0.058 4.8 T014.4-06.1 SB 19 4092512742510443136 279.91691 -19.23682 0.996 0.287 16.046 0.149 0.052 5.3 T011.9-07.4 Kn 78 4079369008737614336 279.97521 -22.05289 0.921 0.103 18.790 0.665 0.276 10.0 P011.1-07.9 SB 17 4079151550306831488 280.08303 -22.90816 0.969 2.034 17.284 0.885 0.137 9.9 L022.1-02.4 M 1-57 4107103777208876928 280.08438 -10.66314 0.973 1.296 15.500 0.220 0.083 6.0 T005.2-10.8 PPA J1840-2931 4047506471715127168 280.21118 -29.52309 0.968 -0.068 19.369 -0.056 0.368 8.5 T023.8-01.7 K 3-11 4155606331827457408 280.28058 -8.93316 0.417 2.039 16.290 0.200 0.064 5.5 T017.9-04.8 M 3-30 4100345805124045696 280.31204 -15.56157 0.984 0.598 17.836 0.249 0.136 9.6 T030.5 + . . . . . . . . . T095.2 + . . . . . . . . . + . . . . . . + + + . . . . . . . . . T032.0 + + . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . + . . . . . . . . . P002.0-13.4 IC 4776 6735622632789070976 281.46131 -33.34285 0.984 -0.190 13.017 . . . . . . . . . . . . . . . . . . + + . . . . . . + . . . P016.0-07.6 SB 21 4098431349179300224 282.04611 -18.49354 1.000 -0.006 18.071 0.280 0.136 12.3 T009.6-10.6 M 3-33 4073217997070348032 282.05056 -25.48125 1.000 -0.230 15.828 0.164 0.054 3.7 T016.7-07.3 SB 22 4098926576110700160 282.12683 -17.73206 0.926 0.447 19.466 -0.224 0.476 3.9 L042.0 + . . . T033.9 + + . . . T029.3-01.2 PHR J1849-0347 4258331057475279616 282.31305 -3.78312 0.246 2.079 16.590 0.745 0.058 38.0 P014.8-08.4 SB 20 4085994773196437888 282.35076 -19.87038 1.000 -0.036 14.986 0.360 0.052 9.5 T026.5-03.0 Pe 1-19 4252307211263954688 282.43605 -7.02649 0.994 0.262 15.881 0.229 0.064 2.2 T051.4 + + + . . . . . . . . . + . . . T025.6-03.6 PM 1-259 4251974334170636416 282.76557 -8.12223 0.828 0.768 14.494 -0.000 0.033 . . .
T026.2-03.4 PHR J1851-0732 4252076348209607296 282.88030 -7.54148 0.743 0.876 18.332 0.225 0.205 22.5 T041.8 + + + + + + . . . + . . . P020.4-07.0 MPA J1854-1420 4101861447517419392 283.56140 -14.33873 0.999 0.167 20.644 . . . . . .
Article number, page 26 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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EDR3
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )024.2-05.2 M 4-11 4202377048194457344 283.57360 -10.08686 0.888 0.314 18.039 0.347 0.159 14.5 T025.3-04.6 K 4-8 4203838127400757248 283.58342 -8.79257 0.993 0.022 16.234 . . . . . . + + + + . . . . . . + + + . . . T016.6-10.5 Kn 55 4085678319975164928 285.14292 -19.23700 0.427 1.374 19.690 -0.141 0.398 . . .
P032.0-03.0 K 3-18 4261880968243745152 285.14510 -2.19946 0.773 2.102 16.928 0.100 0.412 2.0 P017.6-10.2 Abell 51 4086643583803222400 285.25584 -18.20429 1.000 -0.104 15.346 0.552 0.031 29.6 T041.5 + . . . . . . . . . L030.0-04.2 PHR J1901-0429 4254656180365848448 285.31104 -4.49257 0.980 0.294 19.907 0.175 0.571 6.5 T044.4 + + . . . . . . T014.7-11.8 SaWe 4 4081863633097152512 285.57341 -21.44757 0.943 . . . + + + + . . . . . . + . . . . . . . . . + + + + . . . . . . . . . . . . P042.2 + + + + + + . . . . . . . . . + + + . . . . . . + + . . . . . . . . . T019.7-10.7 MPA J1906-1634 4088731114003376512 286.63663 -16.56675 1.000 -0.444 18.412 0.580 0.160 121.0 T042.7 + + + + . . . . . . + + . . . . . . . . . + . . . . . . . . . + . . . . . . . . . . . . L026.8-08.5 Kn 65 4201133736742954880 287.71413 -9.28030 0.997 0.098 18.590 0.203 0.210 30.0 L039.1-02.2 PM 1-285 4293351602342300160 287.72234 4.45786 0.595 2.345 20.939 . . . . . . . . . T Article number, page 27 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )020.9-11.3 PHR J1911-1546 4088900713689049728 287.76863 -15.76875 0.999 -0.414 17.499 0.535 0.130 78.5 T062.4 + + + + . . . P032.1-06.2 FP J1912-0331 4260597185313614976 288.13102 -3.52566 1.000 -0.292 13.992 8.034 0.036 630.0 P040.4-02.0 Pa 129 4293609094235062528 288.17879 5.76284 0.897 1.933 17.687 0.251 0.124 3.0 P048.2 + + . . . . . . . . . + . . . . . . . . . . . . T039.5-02.7 M 2-47 4293191412929039232 288.39393 4.63444 0.920 1.071 16.061 0.201 0.051 3.5 T048.7 + + + + . . . . . . + + . . . . . . + + + + . . . P019.4-13.6 DeHt 3 4084551148755614720 289.26713 -18.02660 1.000 -0.180 20.357 0.692 0.732 16.5 T058.6 + + . . . . . . + . . . L037.5-05.1 Abell 58 4264850714784262272 289.58558 1.78301 0.646 -0.058 20.969 . . . . . . + + . . . + . . . . . . + + . . . + + + . . . . . . . . . P037.7-05.9 PHR J1921 + + + + + + + . . . . . . + . . . T045.4-02.7 Vy 2-2 4308704598615929728 291.09257 9.89893 0.994 1.117 12.776 . . . . . . + + + + . . . P056.0 + . . . . . . . . . + + + + . . . . . . T061.2 + . . . . . . + Article number, page 28 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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EDR3
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )048.1-03.2 IPHASXJ193127.0 + . . . P057.6 + + . . . T047.1-04.2 Abell 62 4314617943916816384 293.32452 10.61656 1.000 -0.025 18.571 0.186 0.213 83.0 T059.4 + + +
30 3639 2032744769234150016 293.68846 30.51634 0.999 0.498 10.337 0.618 0.032 3.1 T053.2-01.5 K 3-38 4322208834752173952 293.82640 17.21682 0.947 . . . . . . . . . . . . + + + + + + + . . . + . . . . . . + + . . . . . . . . . P025.4-16.4 Kn 56 4183190948217334400 294.43240 -13.85566 1.000 -0.296 20.323 1.203 0.633 20.0 T060.5 + + + + + . . . P060.4 + . . . . . . . . . . . . . . . + + . . . P041.4-09.6 Pa 13 4289787771600957824 295.33764 3.12162 1.000 0.131 16.639 0.119 0.058 14.5 T054.4-02.5 M 1-72 1824067323576290304 295.39155 17.75485 0.995 1.211 14.976 0.485 0.345 2.0 T063.2 + + + . . . . . . . . . + + + . . . P057.9-01.5 Hen 2-447 1827414443108647168 296.34234 21.33441 0.996 1.560 17.748 1.030 0.344 1.5 T059.8-00.5 2MASSJ19453289 + . . . . . . + + . . . . . . . . . + . . . P059.7-01.0 IPHASXJ194727.5 + + + + . . . T059.0-01.7 Hen 1-3 1827574864387670400 297.10999 22.14368 0.997 1.224 19.070 -0.272 0.273 4.0 T063.7 + + . . . . . . . . . + + . . . . . . . . . + + . . . . . . . . . Article number, page 29 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )060.3-01.4 IPHASJ194957.59 + . . . . . . . . . . . . + . . . P063.8 + . . . T060.3-02.0 IPHASJ195224.67 + . . . P068.3 + + . . . . . . + + + + + . . . P079.8 + . . . P068.7 + + + + . . . P068.6 + + + + + + . . . P060.0-04.3 Abell 68 1826936121144576896 300.04417 21.71553 0.999 0.616 18.827 0.482 0.187 19.0 T073.0 + + + . . . + . . . T070.9 + . . . P070.2 + + . . . P058.6-05.5 WeSb 5 1823095492701560704 300.42505 19.91115 1.000 0.453 18.114 . . . . . . + . . . . . . . . . . . . + + . . . L046.7-13.7 Pa J2005.8 + + + -7.4 Dr 24 1822392423722386432 302.14089 19.02348 1.000 -0.310 15.009 0.788 0.034 192.0 L079.6 + + + + . . . . . . . . . L064.1-04.9 IPHASXJ201144.3 + + + . . . . . . + Article number, page 30 of 32. Chornay and N. A. Walton: An updated planetary nebula central star catalogue from
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EDR3
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )057.9-09.8 Alves 6 1809885066631267072 303.79164 17.05029 0.998 0.435 13.389 0.597 0.019 150.0 P075.5 + + . . . . . . + + . . . P076.4 + + . . . . . . . . . . . . T073.0-02.4 K 3-76 2055990571034870016 306.27029 33.58068 0.985 1.221 18.004 0.187 0.102 2.1 T089.1 + + + + + + + . . . . . . . . . T072.3-05.3 Kn 23 1862554383714292608 308.60943 31.30901 0.549 0.325 20.253 -0.398 0.605 9.5 T076.3-02.5 MaCCo 2 2056719860792120192 308.81675 36.19729 0.995 1.506 12.654 0.313 0.010 . . .
P097.4 + + + + + + . . . . . . + + . . . . . . + + + + . . . . . . . . . . . . + . . . Article number, page 31 of 32 & A proofs: manuscript no. aanda
Table A.1: continued.
PN G PN name source_id RA Dec reliability BP–RP G ω σ ω PN radius PN status(deg) (deg) (mag) (mag) (mas) (mas) ( (cid:48)(cid:48) )093.4-03.2 StDr 2 1978028088466446848 325.09209 48.36450 1.000 -0.269 17.875 1.552 0.089 18.0 L100.4 + + + + + + + + + . . . P002.7-52.4 IC 5148 /
50 6574225217863069056 329.89623 -39.38566 1.000 -0.585 16.065 0.857 0.053 66.2 T102.5 + + + + . . . . . . + . . . . . . . . . . . . + + + + + + . . . . . . + . . . . . . + -14.9 Dr 21 1938255660503776000 350.95788 45.28171 1.000 -0.345 17.494 0.648 0.095 225.0 T106.5-17.6 NGC 7662 1924818288379268736 351.47430 42.53494 0.997 -0.423 13.930 0.569 0.033 15.2 T111.8-02.8 Hb 12 2009637806507452672 351.56177 58.18182 1.000 0.931 11.771 . . . . . . + + + + + PN status from HASH: T = confirmed PN, L = likely PN, P ==