Table A.1
Observations during EX Lupi quiescence analysed in this paper.
JD | Instrument | Accretion | BC shape |
|
|||
2 454 309.615 | FEROS | M | |
2 454 310.657 | FEROS | M | |
2 454 311.687 | FEROS | L | |
2 454 874.838 | HARPS | H | |
2 454 875.850 | HARPS | H | |
2 454 876.808 | HARPS | M | |
2 454 877.791 | HARPS | M | |
2 454 877.906 | HARPS | L | |
2 454 891.800 | HARPS | H | |
2 454 891.882 | HARPS | H | |
2 454 892.774 | HARPS | M | |
2 454 894.760 | HARPS | L | |
2 455 053.675 | FEROS | L | |
2 455 058.493 | FEROS | M | B |
2 455 257.820 | FEROS | L | |
2 455 259.877 | FEROS | L | |
2 455 262.807 | FEROS | L | |
2 455 263.868 | FEROS | L | |
2 455 309.894 | FEROS | L | |
2 455 338.791 | FEROS | L | |
2 455 353.827 | FEROS | L | |
2 455 396.589 | FEROS | H | C |
2 455 396.637 | FEROS | H | C |
2 455 397.611 | FEROS | M | |
2 455 399.658 | FEROS | M | C |
2 455 400.536 | FEROS | H | B |
2 455 401.506 | FEROS | H | B |
2 455 402.584 | FEROS | M | |
2 455 403.612 | FEROS | M | C |
2 455 405.661 | FEROS | H | C |
2 455 407.620 | FEROS | H | C |
2 455 586.871 | FEROS | H | D |
2 455 587.853 | FEROS | H | C |
2 455 588.858 | FEROS | H | |
2 455 630.816 | FEROS | H | B |
2 455 637.895 | FEROS | M | B |
2 455 667.701 | FEROS | H | |
2 455 668.691 | FEROS | H | D |
2 455 669.737 | FEROS | H | C |
2 455 670.794 | FEROS | H | D |
2 455 671.698 | FEROS | H | C |
2 455 672.876 | FEROS | M | |
2 455 673.849 | FEROS | M | R |
2 455 674.824 | FEROS | H | B |
2 456 111.513 | FEROS | L | |
2 456 113.565 | FEROS | L | |
2 456 114.477 | FEROS | L | R |
2 456 115.477 | FEROS | L | |
2 456 116.524 | FEROS | L | |
2 456 117.562 | FEROS | M | |
2 456 118.670 | FEROS | L | |
2 456 119.494 | FEROS | L | |
2 456 120.508 | FEROS | L | |
2 456 121.579 | FEROS | L |
Notes. The “Accretion” column corresponds to the classification as high/medium/low accretion given in the text, based on the strength of the BC of the emission lines (see Appendix C). The “BC shape” field indicates the shape of the Ca II IR BC, which can be classified as redshifted (R), blueshifted (B), centred (C), or double-peaked (D; see Appendix E). Only spectra with strong BC can be classified (see text).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.