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Table 1.

Gaia DR2 astrometry, photometry, and tangential velocities, initial spectral types from CAFOS spectroscopy, and estimated effective temperatures and our corresponding adopted spectral types of ten new WDs from Gaia colours.

CA No. Alternative Names RAa (degrees) Deca (degrees) Plxa (mas) pmRAa (mas yr−1) pmDeca (mas yr−1) Ga (mag) BP−RPa (mag) Initial SpT Teff (K) Adopted SpT νtanb (km s−1)
037 GD 277 22.350203 +51.145903 26.19 ± 0.05 +32.96 ± 0.09 –110.58 ± 0.09 13.550 –0.338 DA2.5 ± 1.0 22857 ± 2200 DA2.2 ± 0.2 21
054 GD 28 37.170803 +36.760490 24.41 ± 0.06 +10.41 ± 0.10 –171.67 ± 0.08 15.965 +0.292 DA5.0 ± 2.0? 8301 ± 650 DA6.1 ± 0.5 33
078 2MASS J05005185-0930549 75.215835 –9.515829 13.97 ± 0.05 –48.55 ± 0.07 –121.87 ± 0.07 12.616 –0.023 DA3.0 ± 1.5? 11884 ± 1100 DA4.2 ± 0.5 45
082 2MASS J05280449+4105253 82.019148 +41.090348 18.31 ± 0.08 +66.30 ± 0.10 –3.13 ± 0.08 15.124 –0.117 DA3.0 ± 1.0 13994 ± 1100 DA3.6 ± 0.3 17
103 2MASS J07035743+2534184 105.988994 +25.571520 39.06 ± 0.03 –58.29 ± 0.06 –55.69 ± 0.05 13.912 –0.037 DB3.5 ± 1.0? 12168 ± 1100 DB4.1 ± 0.4 10
305 LP 740-47 220.824701 –14.621474 34.89 ± 0.08 –225.37 ± 0.14 –128.43 ± 0.12 16.218 +0.585 DA8.0 ± 1.0 6704 ± 650 DA7.5 ± 0.8 35
376 HD 166435 B 272.331404 +29.956111 40.90 ± 0.04 +66.93 ± 0.06 +74.25 ± 0.07 13.143 –0.344 DA2.5 ± 1.0 23180 ± 2200 DA2.2 ± 0.2 12
397 LSPM J1919+4527 289.900277 +45.463443 35.59 ± 0.04 –108.92 ± 0.08 +312.59 ± 0.09 16.452 +1.194 DC10.5 ± 1.0 4901 ± 300 DC10.3 ± 0.7 44
399 GD 221 291.858997 +10.118643 12.53 ± 0.05 –80.04 ± 0.07 –188.03 ± 0.06 14.724 –0.386 DA2.5 ± 1.0 25771 ± 2200 DA2.0 ± 0.2 77
400 2MASS J19293865+1117523 292.411127 +11.298312 27.34 ± 0.05 +19.15 ± 0.07 +97.83 ± 0.06 13.508 –0.313 DA2.5 ± 1.0 21445 ± 2200 DA2.4 ± 0.3 17

Notes. Gaia DR2 coordinates are for (J2000, epoch 2015.5) and were rounded to 0.000001 degrees, parallaxes and their errors were rounded to 0.01 mas, proper motions and their errors to 0.01 mas yr−1, magnitudes and colours were rounded to 0.001 mag. The initial spectral types with question marks were uncertain because of low S/N or possible problems in the flux calibration of the CAFOS spectra. Further notes on the data:

(a)

Gaia DR2,

(b)

derived from Gaia DR2 parallaxes and proper motions.

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