The GAPS Programme at TNG

@article{Carleo2020TheGP,
  title={The GAPS Programme at TNG},
  author={Ilaria Carleo and Luca Malavolta and Antonino F. Lanza and Mario Damasso and Silvano Desidera and F. Borsa and Matthias Mallonn and Matteo Pinamonti and R. G. Gratton and Eleonora Alei and Serena Benatti and Luigi Mancini and J. Maldonado and K. Biazzo and Massimiliano Esposito and G. Frustagli and E. Gonz{\'a}lez-{\'A}lvarez and Giuseppina Micela and Gaetano Scandariato and Alessandro Sozzetti and L. Affer and A. Bignamini and Aldo S. Bonomo and Riccardo Claudi and Rosario Cosentino and E. Covino and A. F. Martinez Fiorenzano and Paolo Giacobbe and A. Harutyunyan and Giuseppe Leto and Antonio Maggio and E. Molinari and Valerio Nascimbeni and Isabella Pagano and Marco Pedani and Giampaolo Piotto and Ennio Poretti and Monica Rainer and Seth Redfield and Carlo Baffa and A. Baruffolo and Nicolas Buchschacher and V. Billotti and M. Cecconi and Gilberto Falcini and D. Fantinel and Luca Fini and Alberto Galli and A. Ghedina and Francesca Ghinassi and Elisabetta Giani and C. Gonz{\'a}lez and M. Gonzalez and Jos{\'e} Guerra and Marcos Hernandez Diaz and Nauzet Hernandez and Marcella Iuzzolino and Marcello Lodi and Ernesto Oliva and Livia Origlia and H{\'e}ctor P{\'e}rez Ventura and Alfio T. Puglisi and Carlos Riverol and Luis Riverol and J. J. San Juan and Nico Sanna and S. Scuderi and U. Seemann and Mauro Sozzi and Andrea Tozzi},
  journal={Astronomy \& Astrophysics},
  year={2020}
}
Context. The existence of hot Jupiters is still not well understood. Two main channels are thought to be responsible for their current location: a smooth planet migration through the protoplanetary disk or the circularization of an initial highly eccentric orbit by tidal dissipation leading to a strong decrease in the semimajor axis. Different formation scenarios result in different observable effects, such as orbital parameters (obliquity and eccentricity) or frequency of planets at different… 
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We carried out a Bayesian homogeneous determination of the orbital parameters of 231 transiting giant planets (TGPs) that are alone or have distant companions; we employed differential evolution
The GAPS programme with HARPS-N at TNG XI. Pr~0211 in M~44: the first multi-planet system in an open cluster
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The GAPS Programme with HARPS-N at TNG
Aims. In the framework of the GAPS project, we observed the planet-hosting star KELT-9 (A-type star, v sin i ~ 110 km s−1) with the HARPS-N spectrograph at the Telescopio Nazionale Galileo. In this
The HARPS search for southern extra-solar planets - XXXI. The M-dwarf sample
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The GAPS programme with HARPS-N at TNG - I. Observations of the Rossiter-McLaughlin effect and characterisation of the transiting system Qatar-1
Context. Our understanding of the formation and evolution of planetary systems is still fragmentary because most of the current data provide limited information about the orbital structure and
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