Press Release
Open Access

Table K.1.

Table detailing the spectroscopic radial velocity follow-up observations for KIC 10001167.

a BJD-X S/N W rvRG, BF rvMS, BF σRG, BF σMS, BF rvCCF σCCF FWHM con bis MS
8385.4869 49 0.7 -92.749 -113.420 0.095 0.515 -92.266 0.091 9.364 21.138 0.1406 1
8386.4297 41 0.6 -93.561 -113.090 0.095 0.750 -93.080 0.091 9.394 21.022 0.0954 1
8386.4521 49 0.7 -93.618 -113.077 0.096 0.482 -93.144 0.091 9.425 21.158 0.1590 0
8392.4546 60 0 -99.187 0.096 -98.731 0.091 9.302 21.460 0.1362 0
8393.4032 58 0 -100.132 0.096 -99.642 0.091 9.348 21.166 0.1430 0
8396.3671 46 0 -103.213 0.098 -102.737 0.091 9.528 21.332 0.1555 0
8407.4649 52 0 -116.255 -88.007 0.097 0.485 -115.788 0.091 9.242 20.938 0.1507 1
8426.3591 54 0.7 -131.251 -71.169 0.095 0.145 -130.763 0.091 9.388 20.951 0.1358 1
8427.3655 57 0.7 -131.181 -70.365 0.097 0.549 -130.704 0.090 9.367 20.965 0.1043 1
8428.4015 41 0.7 -131.074 -71.323 0.097 0.329 -130.569 0.091 9.533 20.842 0.1139 1
8429.3965 45 0.7 -130.792 -72.091 0.096 0.373 -130.307 0.091 9.346 20.985 0.1244 1
8437.3641 53 0.7 -124.212 -78.969 0.096 0.270 -123.739 0.091 9.408 20.919 0.1547 1
8446.3035 49 0 -110.724 -94.231 0.096 0.466 -110.236 0.091 9.598 20.861 0.1646 0
8454.3115 54 0 -98.399 0.096 -97.943 0.091 9.303 21.063 0.1308 0
8458.3207 19 0.7 -93.362 -113.348 0.098 0.932 -92.868 0.098 9.247 20.366 0.2036 0
8461.3147 31 0.7 -90.055 -117.316 0.094 0.887 -89.628 0.092 9.300 20.792 0.1831 1
9036.5826 70 1 -127.251 -75.462 0.094 0.228 -126.791 0.091 9.225 21.034 0.1368 1
9037.6167 49 1 -126.145 -77.410 0.094 0.694 -125.718 0.091 9.446 21.0786 0.1349 1
9038.5733 62 1 -125.039 -78.325 0.095 0.462 -124.585 0.091 9.362 21.178 0.1502 1
9039.6590 64 1 -123.758 -79.740 0.094 0.361 -123.336 0.091 9.358 21.191 0.1431 1
9047.5846 11 0 -111.847 -91.784 0.113 1.432 -111.314 0.129 10.201 20.820 0.1699 0
9072.5926 84 1 -83.571 -124.487 0.096 0.560 -83.100 0.091 9.193 20.897 0.1915 1
9077.5191 85 1 -81.939 -125.561 0.096 0.248 -81.505 0.091 9.088 21.135 0.1724 1
9078.5015 88 1 -81.747 -126.538 0.096 0.430 -81.312 0.090 9.242 21.180 0.1424 1
9079.5529 78 1 -81.597 -126.711 0.097 0.449 -81.155 0.090 9.254 21.181 0.1573 1
9082.3838 86 1 -81.402 -127.040 0.095 0.349 -80.976 0.090 9.106 21.109 0.1405 1
9380.5590 63 0.9 -127.003 -76.544 0.095 0.332 -126.538 0.091 9.248 21.081 0.1776 1
9429.4490 44 0.7 -86.068 -121.504 0.094 0.608 -85.594 0.091 9.387 20.671 0.1456 1
9433.5892 54 0.7 -83.692 -124.280 0.096 0.461 -83.250 0.091 9.392 20.690 0.1399 1
9446.5612 78 0.9 -81.757 -126.571 0.096 0.554 -81.331 0.090 9.185 20.639 0.1370 1
9863.4595 56 0.7 -128.353 -74.807 0.096 0.258 -127.918 0.091 9.079 20.677 0.1590 1
9989.7557 27 0 -131.301 -70.671 0.098 0.792 -130.886 0.093 9.370 20.538 0.2043 0
9996.7724 36 0 -129.837 -72.915 0.095 0.355 -129.376 0.091 9.194 20.542 0.1681 1
10002.7624 53 0 -123.889 -79.214 0.094 0.328 -123.474 0.091 9.320 20.646 0.1718 1
10007.7233 46 0 -116.626 -87.391 0.095 0.733 -116.187 0.091 9.217 20.727 0.1458 1
10015.6930 41 0 -103.809 0.096 -103.343 0.091 9.451 21.187 0.1900 0
10021.7254 53 0 -95.333 -111.835 0.096 0.375 -94.892 0.091 9.167 21.100 0.1919 0
10032.7096 23 0 -84.995 0.098 -84.521 0.094 9.616 20.694 0.2135 0
10033.6893 16 0 -84.393 0.105 -83.995 0.099 8.974 20.751 0.1825 0
10033.7385 21 0 -84.366 0.100 -83.888 0.093 9.141 20.875 0.0977 1
10036.6912 37 0 -82.951 0.097 -82.495 0.091 9.439 20.765 0.1516 1
10042.6514 63 0 -81.460 -126.517 0.095 0.344 -80.995 0.091 9.292 20.677 0.1585 1
10047.6683 33 0 -81.385 -127.532 0.097 0.537 -80.943 0.091 9.714 20.521 0.1500 1
10061.5616 48 0 -86.226 -121.694 0.094 0.288 -85.799 0.097 9.787 20.617 0.1626 1
10069.6970 58 0 -91.893 -115.821 0.096 0.623 -91.457 0.098 9.240 20.694 0.1819 1
(a)

Notes. Columns, and their units, are as follows: BJD-X is the barycentric julian date - 2450000. S/N is estimated Signal/Noise ratio of the full frame images at ∼5880Å. W is the weight applied to each spectrum when performing the spectral separation. rvRG, BF and rvMS, BF [km/s] are the radial velocities of the giant and main sequence star from the main broadening function analysis. σRG, BF and σMS, BF [km/s] are the corresponding RV uncertainties for the giant and main sequence star used in the eclipsing binary analysis. Similar results are reported for the independent CCF analysis of the RG. For that analysis, we also carried out full-width at half maximum (FWHM) [km/s], line contrast (con), and bisector-span (bis) measurements. Last, the spectra included for MS component fit with the CCF method is reported in (MS).

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.