Table 1.
Members of the (36256) 1999 XT17 family with a Gaia DR3 spectrum.
| Asteroid | D | pV | Avg | H | Spectral |
|---|---|---|---|---|---|
| Number | (km) | S/N | class | ||
| 15610 | 5.84 | 0.30 | 35.32 | 13.3 | A, L |
| 16789 | 6.62 | 0.18 | 38.25 | 13.5 | A, Sv |
| 20975 | 5.24 | 0.28 | 36.01 | 13.6 | A, Sv |
| 25356 | – | – | 66.49 | 12.8 | A, Sa |
| 27565 | 5.92 | 0.19 | 20.74 | 13.6 | A, L |
| 33763 | – | – | 48.07 | 13.4 | A, Sa |
| 34902 | 4.15 | 0.15 | 14.7 | 14.4 | Sq, Sr |
| 36256 | 10.21 | 0.19 | 66.56 | 12.4 | A, Sa |
| 40671 | – | – | 28.09 | 13.6 | A, Sa |
| 57276 | 7.20 | 0.31 | 128.7 | 12.9 | A, Sv |
| 66676 | 6.55 | 0.22 | 52.28 | 13.3 | L, A |
| 83124 | – | – | 14.88 | 14.7 | S, Sr |
| 88057 | – | – | 20.75 | 14.5 | K, S |
| 99004 | 3.83 | 0.10 | 13.93 | 14.6 | L, A |
| 140349 | 3.69 | 0.20 | 13.86 | 14.7 | Sv, A |
Notes. Here is given the diameter D of family members, their geometric visible albedo pV, the average signal-to-noise ratio of their DR3 spectrum S/N, their H magnitude, and the two best spectral classes given by our classification algorithm. The physical properties data were obtained from http://mp3c.oca.eu/.
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