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Table 5.
Measured parameters of the stars observed with LAMOST.
| Gaia DR3 | Teff (K) | log(g) | SpT_tw | SpT_lit |
|---|---|---|---|---|
| 3377027132948376704 | 13 500 ± 500 | 3.75 ± 0.25 | B7 ± 1IV | – |
| 3377026961149682432 | 16 000 ± 1000 | 4.25 ± 0.25 | B4 ± 1V | – |
| 3377004215002923904 | 19 000 ± 1000 | 4.25 ± 0.25 | B2.5 ± 0.5V | – |
| 3377002840613390592 | 11 500 ± 500 | 4.00 ± 0.25 | B9 ± 1V | – |
| 3376999709578280064 | 25 000 ± 2000 | 4.25 ± 0.25 | B0.5 ± 0.5V | B2/3 III (1) |
| 3377029950446864896 | 15 000 ± 1000 | 4.25 ± 0.25 | B5 ± 1V | – |
| 3377054620738994816 | 10 000 ± 500 | 3.00 ± 0.25 | B9.5 ± 0.5III | – |
| 3377012731919116416 | 26 000 ± 2000 | 4.25 ± 0.25 | B0.5 ± 0.5V | B8 (2) |
| 3377012697559377664 | 15 000 ± 1000 | 4.25 ± 0.25 | B5 ± 1V | – |
| 3377049737357365760 | 15 000 ± 1000 | 4.25 ± 0.25 | B5 ± 1IV | – |
| 3377037230412601472 | 10 000 ± 500 | 2.75 ± 0.25 | B9.5 ± 0.5II | – |
| 3377039433734571520 | 15 000 ± 1000 | 4.25 ± 0.25 | B5 ± 1IV | – |
| 3377044690774512896 | 20 000 ± 2000 | 4.25 ± 0.25 | B2 ± 1V | – |
| 3377046168243238528 | 13 000 ± 500 | 4.25 ± 0.25 | B7 ± 1V | – |
| 3377033936176712192 | 12 000 ± 500 | 3.50 ± 0.25 | B8 ± 1IV | – |
| 3377040464526993920 | 19 000 ± 1000 | 4.25 ± 0.25 | B2.5 ± 0.5V | – |
| 3376852070081305344 | 10 000 ± 500 | 4.00 ± 0.25 | B9.5 ± 0.5IV | – |
Notes. The spectral types suggested for the stars in this work (SpT_tw), with the most precise determination available in the literature (SpT_lit), are given. (1) Crawford et al. (1955) and (2) Fabricius et al. (2002).
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