Re-assessing the radial-velocity evidence for planets around CoRoT-7
CoRoT-7 is an 11th magnitude K-star whose light curve shows transits with depth of 0.3 mmag and a period of 0.854 d, superimposed on variability at the 1% level, due to the modulation of evolving active regions with the star's 23 d rotation period. In this paper, we revisit the published HARPS...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2010
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