A CHEOPS-enhanced view of the HD 3167 system
- Bourrier, V.
- Deline, A.
- Krenn, A.
- Egger, J.A.
- Petit, A.C.
- Malavolta, L.
- Cretignier, M.
- Billot, N.
- Broeg, C.
- Florén, H.-G.
- Queloz, D.
- Alibert, Y.
- Bonfanti, A.
- Bonomo, A.S.
- Delisle, J.-B.
- Demangeon, O.D.S.
- Demory, B.-O.
- Dumusque, X.
- Ehrenreich, D.
- Haywood, R.D.
- Howell, S.B.
- Lendl, M.
- Mortier, A.
- Nigro, G.
- Salmon, S.
- Sousa, S.G.
- Wilson, T.G.
- Adibekyan, V.
- Alonso, R.
- Anglada, G.
- Bárczy, T.
- Barrado Y Navascues, D.
- Barros, S.C.C.
- Baumjohann, W.
- Beck, M.
- Benz, W.
- Biondi, F.
- Bonfils, X.
- Brandeker, A.
- Cabrera, J.
- Charnoz, S.
- Csizmadia, S.
- Collier Cameron, A.
- Damasso, M.
- Davies, M.B.
- Deleuil, M.
- Delrez, L.
- Di Fabrizio, L.
- Erikson, A.
- Fortier, A.
- Fossati, L.
- Fridlund, M.
- Gandolfi, D.
- Gillon, M.
- Güdel, M.
- Heng, K.
- Hoyer, S.
- Isaak, K.G.
- Kiss, L.L.
- Laskar, J.
- Lecavelier Des Etangs, A.
- Lorenzi, V.
- Lovis, C.
- Magrin, D.
- Massa, A.
- Maxted, P.F.L.
- Nascimbeni, V.
- Olofsson, G.
- Ottensamer, R.
- Pagano, I.
- Pallé, E.
- Peter, G.
- Piotto, G.
- Pollacco, D.
- Ragazzoni, R.
- Rando, N.
- Rauer, H.
- Ribas, I.
- Santos, N.C.
- Scandariato, G.
- Ségransan, D.
- Simon, A.E.
- Smith, A.M.S.
- Steller, M.
- Szabó, G.M.
- Thomas, N.
- Udry, S.
- Van Grootel, V.
- Verrecchia, F.
- Walton, N.
- Beck, T.
- Buder, M.
- Ratti, F.
- Ulmer, B.
- Viotto, V.
DOIAbstract
A. C. C. and T. G. W. acknowledge support from STFC consolidated grant numbers ST/R000824/1 and ST/V000861/1, and UKSA grant number ST/R003203/1.Much remains to be understood about the nature of exoplanets smaller than Neptune, most of which have been discovered in compact multi-planet systems. With its inner ultra-short period planet b aligned with the star and two larger outer planets d-c on polar orbits, the multi-planet system HD 3167 features a peculiar architecture and offers the possibility to investigate both dynamical and atmospheric evolution processes. To this purpose we combined multiple datasets of transit photometry and radial velocimetry (RV) to revise the properties of the system and inform models of its planets. This effort...
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