| 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. | 3 |
| 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 of O'Brien et al. (2024).
Mairi O'Brien, Department of Physics, University of Warwick, Coventry CV4 7AL, UK