| csv file | Description | Version |
|---|---|---|
| Table A1 | The catalogue of 1078 Gaia white dwarfs within 40 pc. See Table 1 of O'Brien et al. (2024) for header descriptions. | 2 |
| Table A2 | White dwarf candidates within 40 pc in the Gentile Fusillo et al. (2021) DR3 catalogue that do not have spectroscopic follow-up. | 2 |
| Table A3 | Confirmed white dwarfs and candidates in the Gentile Fusillo et al. (2021) DR3 catalogue that are within 1 sigma of 40 pc. | 1 |
| Table A4 | White dwarfs that are not in the Gentile Fusillo et al. (2021) DR3 catalogue. | 1 |
| Table A5 | White dwarfs within 40 pc with unreliable Gaia parameters. Best-fit parameters are instead taken from literature. | 1 |
| Table A6 | List of wide binaries and higher-order systems, where at least one companion is a white dwarf, within 40 pc. The projected separation between sources is given in pc and au, and the tangential velocity difference is in km/s. | 1 |
| Contaminants | List of confirmed main-sequence contaminants to the 40 pc white dwarf sample. | 1 |
Notes: Three new white dwarfs have been confirmed spectroscopically following publication. Corrected cooling ages have been removed from Table A1, these can be calculated using Bedard et al. (2020) cooling models.
Mairi O'Brien, Department of Physics, University of Warwick, Coventry CV4 7AL, UK