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Table A.1.
Journal of the observations of HR 6819.
HJD [d] | Time [s] | S/N | RV1 [km s−1] |
---|---|---|---|
2451373.676 | 300 | 150 | −39.0 ± 4.5 |
2451374.675 | 300 | 290 | −43.6 ± 4.5 |
2451375.653 | 300 | 300 | −41.6 ± 4.5 |
2451376.724 | 1800 | 200 | −30.9 ± 4.5 |
2451378.682 | 1500 | 280 | −27.7 ± 4.4 |
2451380.824 | 360 | 240 | −14.8 ± 4.4 |
2451383.673 | 300 | 270 | 12.1 ± 4.4 |
2451384.743 | 300 | 230 | 24.1 ± 4.4 |
2451385.759 | 300 | 200 | 32.8 ± 4.5 |
2451390.745 | 300 | 300 | 62.9 ± 4.9 |
2451393.627 | 300 | 200 | 68.9 ± 5.1 |
2451394.758 | 300 | 220 | 65.5 ± 5.0 |
2453138.847 | 150 | 320 | −7.7 ± 4.4 |
2453139.682 | 150 | 300 | −14.5 ± 4.4 |
2453143.808 | 150 | 230 | −50.0 ± 4.6 |
2453144.753 | 150 | 340 | −54.4 ± 4.6 |
2453149.762 | 150 | 320 | −51.1 ± 4.6 |
2453149.765 | 150 | 320 | −51.1 ± 4.6 |
2453154.669 | 150 | 300 | −21.5 ± 4.4 |
2453159.804 | 150 | 340 | 18.5 ± 4.4 |
2453160.686 | 150 | 370 | 28.5 ± 4.5 |
2453162.862 | 150 | 230 | 42.0 ± 4.5 |
2453185.551 | 150 | 400 | −52.6 ± 4.6 |
2453187.666 | 150 | 330 | −51.6 ± 4.6 |
2453188.687 | 150 | 360 | −53.7 ± 4.6 |
2453190.704 | 150 | 310 | −49.3 ± 4.6 |
2453194.691 | 150 | 350 | −25.6 ± 4.4 |
2453195.563 | 150 | 350 | −14.7 ± 4.4 |
2453196.550 | 150 | 270 | −2.7 ± 4.4 |
2453197.670 | 150 | 330 | 8.1 ± 4.4 |
2453199.570 | 150 | 310 | 26.8 ± 4.5 |
2453202.645 | 150 | 330 | 51.4 ± 4.7 |
2453204.513 | 150 | 340 | 66.3 ± 5.0 |
2453205.697 | 150 | 320 | 69.8 ± 5.2 |
2453207.501 | 150 | 250 | 74.9 ± 5.3 |
2453226.596 | 150 | 290 | −52.0 ± 4.6 |
2453230.490 | 150 | 420 | −45.9 ± 4.5 |
2453231.569 | 150 | 360 | −40.5 ± 4.5 |
2453232.502 | 150 | 300 | −39.7 ± 4.5 |
2453239.494 | 150 | 420 | 21.2 ± 4.4 |
2453240.602 | 150 | 300 | 29.6 ± 4.5 |
2453243.515 | 150 | 400 | 56.9 ± 4.8 |
2453244.551 | 150 | 370 | 62.4 ± 4.9 |
2453245.510 | 150 | 430 | 67.0 ± 5.1 |
2453246.619 | 150 | 310 | 64.7 ± 5.0 |
2453247.553 | 150 | 320 | 64.4 ± 5.0 |
2453248.522 | 150 | 430 | 69.4 ± 5.1 |
2453254.539 | 150 | 300 | 48.0 ± 4.6 |
2453255.515 | 150 | 290 | 36.5 ± 4.5 |
2453256.555 | 150 | 250 | 27.7 ± 4.5 |
2453257.534 | 150 | 350 | 21.0 ± 4.4 |
2453258.492 | 150 | 350 | 16.3 ± 4.4 |
2453259.531 | 150 | 400 | 3.6 ± 4.4 |
2453260.536 | 150 | 380 | −5.3 ± 4.4 |
2453261.541 | 150 | 370 | −13.7 ± 4.4 |
2453262.530 | 150 | 400 | −21.3 ± 4.4 |
2453263.536 | 150 | 420 | −35.7 ± 4.5 |
2453264.567 | 150 | 340 | −42.6 ± 4.5 |
2453264.567 | 150 | 340 | −42.6 ± 4.5 |
2453265.490 | 150 | 370 | −44.8 ± 4.5 |
2453269.508 | 150 | 310 | −52.2 ± 4.6 |
2453271.514 | 150 | 310 | −44.7 ± 4.5 |
2453272.540 | 150 | 410 | −37.5 ± 4.5 |
2453273.505 | 150 | 360 | −28.7 ± 4.4 |
Notes. The second column indicates the exposure time while the third column gives the S/N ratio in the spectrum at ≈5400 Å. The last column gives the RV of the primary star.
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