Table A.1
Journal of our new optical spectra of 9 Sgr.
| HJD-2 450 000 | Exp. time | Instrument | RV1 | σ 1 | RV2 | σ 2 | |
| (s) | (km s-1) | (km s-1) | (km s-1) | (km s-1) | |||
|
|
|||||||
| 4995.5949 | 360 | H | 10.6 | 19.3 | 14.6 | 3.7 | |
| 5017.4735 | 1200 | H | 10.5 | 9.3 | 13.2 | 1.9 | |
| 5037.4475 | 720 | H | 15.4 | 10.1 | 12.7 | 4.0 | |
| 5080.3962 | 2500 | H | 13.7 | 2.4 | 13.0 | 4.1 | |
| 5101.3382 | 360 | H | 16.6 | 6.1 | 12.5 | 2.1 | |
| 5291.7128 | 900 | H | 15.3 | 6.8 | 14.1 | 2.3 | |
| 5334.6592 | 800 | H | 14.0 | 4.2 | 10.9 | 1.4 | |
| 5342.6792 | 1200 | H | 13.8 | 4.3 | 10.5 | 2.0 | |
| 5377.4840 | 900 | H | 15.0 | 8.6 | 9.6 | 2.8 | |
| 5430.3849 | 960 | H | 12.5 | 6.4 | 9.0 | 2.8 | |
| 5660.7078 | 600 | H | 18.3 | 5.7 | 6.6 | 2.8 | |
| 5684.6663 | 600 | H | 16.8 | 9.4 | 6.6 | 1.8 | |
| 5703.6817 | 2160 | H | 13.9 | 1.7 | 6.9 | 2.6 | |
| 5704.6231 | 2160 | H | 16.1 | 3.4 | 6.4 | 2.2 | |
| 5705.5434 | 720 | H | 19.6 | 12.9 | 4.9 | 5.7 | |
| 5748.5052 | 360 | H | 24.6 | 2.6 | 4.9 | 2.2 | |
| 5750.4500 | 360 | H | 21.1 | 10.0 | 3.9 | 3.1 | |
| 5769.5233 | 1200 | H | 16.2 | 7.2 | 5.6 | 1.5 | |
| 5790.4075 | 460 | H | 21.0 | 4.8 | 1.6 | 5.6 | |
| 5795.4051 | 500 | H | 18.9 | 2.1 | 4.9 | 3.0 | |
| 6038.7276 | 1080 | H | 23.8 | 4.0 | −1.6 | 2.5 | |
| 6052.9305 | 300 | F | 22.0 | 18.5 | −1.9 | 4.6 | |
| 6053.6602 | 360 | H | 26.1 | 4.1 | −1.0 | 5.1 | |
| 6069.6341 | 360 | H | 26.8 | 8.9 | −5.7 | 6.2 | |
| 6111.5867 | 360 | H | 26.4 | 3.6 | −3.3 | 4.4 | |
| 6125.4789 | 360 | H | 25.8 | 6.2 | −5.7 | 4.0 | |
| 6126.4975 | 600 | H | 25.0 | 7.7 | −3.7 | 5.0 | |
| 6146.4494 | 360 | H | 20.9 | 7.5 | −12.6 | 11.1 | |
| 6171.5517 | 600 | C | 27.5 | 3.7 | −13.9 | 4.3 | |
| 6218.4937 | 650 | C | 32.5 | 8.3 | −16.2 | 2.2 | |
| 6354.8983 | 623 | C | 31.3 | 8.3 | −31.6 | 6.2 | |
| 6420.6492 | 480 | H | 46.1 | 16.5 | −45.5 | 10.8 | |
| 6431.8842 | 623 | C | 40.4 | 13.0 | −48.4 | 4.1 | |
| 6458.6064 | 600 | C | 56.2 | 11.2 | −53.9 | 4.6 | |
| 6461.5358 | 360 | H | 52.9 | 19.2 | −53.4 | 10.2 | |
| 6463.5440 | 360 | H | 50.9 | 17.7 | −52.9 | 10.0 | |
| 6508.6147 | 623 | C | 54.5 | 11.9 | −57.4 | 6.1 | |
| 6513.3831 | 690 | H | 57.7 | 8.7 | −53.8 | 9.5 | |
| 6544.5270 | 600 | C | 46.7 | 10.8 | −54.1 | 8.0 | |
| 6808.6165 | 360 | H | 9.3 | 5.6 | 7.7 | 8.0 | |
| 6829.5383 | 360 | H | 5.7 | 1.7 | 12.4 | 2.4 | |
| 6846.4309 | 360 | H | 17.6 | 19.2 | 12.6 | 1.8 | |
| 6878.4413 | 360 | H | 11.7 | 5.0 | 12.7 | 1.1 | |
| 6879.4112 | 360 | H | 9.3 | 7.3 | 13.0 | 2.0 | |
| 6900.3964 | 620 | H | −1.4 | 11.0 | 14.2 | 1.4 | |
| 7156.6508 | 1800 | H | 6.0 | 9.8 | 17.3 | 3.4 | |
Notes. The codes for the instrument correspond to HERMES (H), FEROS (F) and Coralie (C). The columns labelled σ1 and σ2 provide the 1σ dispersion about the mean RV of the various lines (corrected for systematic shifts) used to evaluate the RV of the primary and secondary, respectively.
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