Table C.1
Radial velocity results.
| Object | MJD | RV | Err | Template | υ sin i | Qual. | Comment |
|---|---|---|---|---|---|---|---|
| (km s−1) | (km s−1) | PoWR model | (km s−1) | ||||
| AV-6 | 59149.305 | 154.9 | 0.4 | smc-ob-i_33-38 | 50 | 5 | |
| AV-14 | 59156.195 | 144.1 | 0.8 | smc-ob-i_43-40 | 150 | 5 | XB (Simbad) |
| AV-15 | 59155.047 | 128.5 | 0.5 | smc-ob-ii_38-36 | 100 | 5 | |
| AV-18 | 59155.058 | 152.2 | 0.4 | smc-ob-iii_20-26 | 50 | 6 | |
| AV-22 | 59155.012 | 140.4 | 0.3 | smc-ob-i_16-22 | 50 | 5 | |
| AV-43 | 59157.252 | 168.7 | 1.0 | smc-ob-i_24-32 | 250 | 3 | |
| 59157.261 | 168.2 | 1.0 | smc-ob-i_24-32 | 250 | 3 | ||
| — | — | — | — | — | — | — | — |
Notes. Column 1: object identifier (a given star can have multiple entries if there are multiple observations more than 15 min apart). Col 2: Modified Julian Date (MJD) of the start of observation; Col. 3: Radial velocity (RV); Col. 4: RV uncertainty (an underestimate in most cases); Col. 5: Code of the template PoWR model used; Col. 6: Projected rotational velocity (υ sin i) used in the cross-correlation; Col. 7: Quality of the fit (range 0 – 8), where low values indicate a bad quality and high values a good quality; Col. 8: Comments about possible binarity, mostly from Simbad. EB=eclipsing binary, XB=X-ray binary. The full table is available at CDS.
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