Free Access

Table 12

Characterization of candidates around M-dwarfs, according to the analytic transit fit.

Candidate Period (days) t 0 i(°) Rplanet(RJup) Rplanet,min(RJup) Rplanet,max(RJup) Classification

19b4-10711 1.55274390 2 454 318.1664350 85.16 2.53 2.34 2.84 1.28 B
19e3-01290 2.46752082 2 454 318.6477813 85.86 2.64 2.34 3.20 1.01 B
19a2-10046 1.45677364 2 454 318.7173035 84.48 2.78 2.46 5.31 1.43 B
19a1-02980 1.05176697 2 454 318.6516446 72.80 3.25 1.93 6.95 1.31 B
19a1-07499 1.96038974 2 454 318.5897989 81.29 3.45 2.14 7.28 1.18 B
19e3-05850 9.20198442 2 454 320.1712614 86.81 3.48 3.30 5.03 1.06 B
19a1-10878 1.55498531 2 454 317.9578553 83.43 3.71 3.49 3.99 1.32 B
19a1-01358 1.10712079 2 454 318.6005745 76.76 4.94 1.71 7.12 1.09 B

Notes. Orbital and planetary parameters derived from the analytic transit model fit. All candidates are too large and are most likely transiting brown dwarfs or low-mass stars.

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.